Mass Distribution and Maximum Mass of Neutron Stars: Effects of Orbital Inclination Angle
Matter at ultra-high densities finds a physical realization inside neutron stars. One key property is their maximum mass, which has far-reaching implications for astrophysics and the equation of state of ultra dense matter. In this work, we employ Bayesian analysis to scrutinize the mass distributio...
Saved in:
Published in | Universe (Basel) Vol. 10; no. 1; p. 3 |
---|---|
Main Authors | , , , , , |
Format | Journal Article |
Language | English |
Published |
Basel
MDPI AG
01.01.2024
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Abstract | Matter at ultra-high densities finds a physical realization inside neutron stars. One key property is their maximum mass, which has far-reaching implications for astrophysics and the equation of state of ultra dense matter. In this work, we employ Bayesian analysis to scrutinize the mass distribution and maximum mass threshold of galactic neutron stars. We compare two distinct models to assess the impact of assuming a uniform distribution for the most important quantity, the cosine of orbital inclination angles (i), which has been a common practice in previous analyses. This prevailing assumption yields a maximum mass of 2.25 M⊙ (2.15–3.32 M⊙ within 90% confidence), with a strong peak around the maximum value. However, in the second model, which indirectly includes observational constraints of i, the analysis supports a mass limit of 2.56−0.58+0.87M⊙ (2σ uncertainty), a result that points in the same direction as some recent results gathered from gravitational wave observations, although their statistics are still limited. This work stresses the importance of an accurate treatment of orbital inclination angles, and contributes to the ongoing debate about the maximum neutron star mass, further emphasizing the critical role of uncertainties in the individual neutron star mass determinations. |
---|---|
AbstractList | Matter at ultra-high densities finds a physical realization inside neutron stars. One key property is their maximum mass, which has far-reaching implications for astrophysics and the equation of state of ultra dense matter. In this work, we employ Bayesian analysis to scrutinize the mass distribution and maximum mass threshold of galactic neutron stars. We compare two distinct models to assess the impact of assuming a uniform distribution for the most important quantity, the cosine of orbital inclination angles (i), which has been a common practice in previous analyses. This prevailing assumption yields a maximum mass of 2.25 M[sub.⊙] (2.15–3.32 M[sub.⊙] within 90% confidence), with a strong peak around the maximum value. However, in the second model, which indirectly includes observational constraints of i, the analysis supports a mass limit of 2.56[sub.−0.58] [sup.+0.87] M[sub.⊙] (2σ uncertainty), a result that points in the same direction as some recent results gathered from gravitational wave observations, although their statistics are still limited. This work stresses the importance of an accurate treatment of orbital inclination angles, and contributes to the ongoing debate about the maximum neutron star mass, further emphasizing the critical role of uncertainties in the individual neutron star mass determinations. Matter at ultra-high densities finds a physical realization inside neutron stars. One key property is their maximum mass, which has far-reaching implications for astrophysics and the equation of state of ultra dense matter. In this work, we employ Bayesian analysis to scrutinize the mass distribution and maximum mass threshold of galactic neutron stars. We compare two distinct models to assess the impact of assuming a uniform distribution for the most important quantity, the cosine of orbital inclination angles (i), which has been a common practice in previous analyses. This prevailing assumption yields a maximum mass of 2.25 M⊙ (2.15–3.32 M⊙ within 90% confidence), with a strong peak around the maximum value. However, in the second model, which indirectly includes observational constraints of i, the analysis supports a mass limit of 2.56−0.58+0.87M⊙ (2σ uncertainty), a result that points in the same direction as some recent results gathered from gravitational wave observations, although their statistics are still limited. This work stresses the importance of an accurate treatment of orbital inclination angles, and contributes to the ongoing debate about the maximum neutron star mass, further emphasizing the critical role of uncertainties in the individual neutron star mass determinations. Matter at ultra-high densities finds a physical realization inside neutron stars. One key property is their maximum mass, which has far-reaching implications for astrophysics and the equation of state of ultra dense matter. In this work, we employ Bayesian analysis to scrutinize the mass distribution and maximum mass threshold of galactic neutron stars. We compare two distinct models to assess the impact of assuming a uniform distribution for the most important quantity, the cosine of orbital inclination angles (i), which has been a common practice in previous analyses. This prevailing assumption yields a maximum mass of 2.25 M⊙ (2.15–3.32 M⊙ within 90% confidence), with a strong peak around the maximum value. However, in the second model, which indirectly includes observational constraints of i, the analysis supports a mass limit of 2.56−0.58+0.87M⊙ (2σ uncertainty), a result that points in the same direction as some recent results gathered from gravitational wave observations, although their statistics are still limited. This work stresses the importance of an accurate treatment of orbital inclination angles, and contributes to the ongoing debate about the maximum neutron star mass, further emphasizing the critical role of uncertainties in the individual neutron star mass determinations. Matter at ultra-high densities finds a physical realization inside neutron stars. One key property is their maximum mass, which has far-reaching implications for astrophysics and the equation of state of ultra dense matter. In this work, we employ Bayesian analysis to scrutinize the mass distribution and maximum mass threshold of galactic neutron stars. We compare two distinct models to assess the impact of assuming a uniform distribution for the most important quantity, the cosine of orbital inclination angles (i), which has been a common practice in previous analyses. This prevailing assumption yields a maximum mass of 2.25 M⊙ (2.15–3.32 M⊙ within 90% confidence), with a strong peak around the maximum value. However, in the second model, which indirectly includes observational constraints of i, the analysis supports a mass limit of 2.56−0.58+0.87 M⊙ ( 2σ uncertainty), a result that points in the same direction as some recent results gathered from gravitational wave observations, although their statistics are still limited. This work stresses the importance of an accurate treatment of orbital inclination angles, and contributes to the ongoing debate about the maximum neutron star mass, further emphasizing the critical role of uncertainties in the individual neutron star mass determinations. |
Audience | Academic |
Author | Barão, Lucas G. Horvath, Jorge E. de Avellar, Marcio G. B. Rocha, Lívia S. de Sá, Lucas M. Chinen, Gustavo Y. |
Author_xml | – sequence: 1 givenname: Lívia S. orcidid: 0000-0003-4543-0912 surname: Rocha fullname: Rocha, Lívia S. – sequence: 2 givenname: Jorge E. orcidid: 0000-0003-4089-3440 surname: Horvath fullname: Horvath, Jorge E. – sequence: 3 givenname: Lucas M. orcidid: 0000-0003-3109-9042 surname: de Sá fullname: de Sá, Lucas M. – sequence: 4 givenname: Gustavo Y. orcidid: 0009-0009-4458-8268 surname: Chinen fullname: Chinen, Gustavo Y. – sequence: 5 givenname: Lucas G. orcidid: 0009-0000-3268-9058 surname: Barão fullname: Barão, Lucas G. – sequence: 6 givenname: Marcio G. B. orcidid: 0000-0003-1771-1055 surname: de Avellar fullname: de Avellar, Marcio G. B. |
BookMark | eNpdUU1rGzEQFSWFJk7uPS7k7FRfu5J6M_loDfk4NDn0JEZaycispUTShvTfV7VLKEUDmpn35jHDO0FHMUWH0GeCLxhT-Mscw6vLxRGMW2D2AR1TSuSSKCWO_sk_obNSto1BRN9KeYx-3kEp3VUoNQcz15BiB3Hs7uAt7OZdt0eT7-7dXHPDflTI5Wt37b2zdY88ZBMqTN062ilE2Cus4mZyp-ijh6m4s7__Aj3dXD9efl_ePnxbX65ul5YJUpeup1Rw4y0bqCHtAo4NNcIAwXIQfS-pVT0IbpUj3IhRDZIZyTHwdrngI1ug9UF3TLDVzznsIP_SCYLeN1LeaMg12MlpBXZwnBLTY88NGRTGVnHCeA-qH61sWucHreecXmZXqt6mOce2vqaKSKGYEKyxLg6sDTTREH2qGWx7o9sF25zxofVXQmJFJeWqDeDDgM2plOz8-5oE6z8G6v8NZL8BpfSPMQ |
Cites_doi | 10.1051/0004-6361/201015532 10.3390/galaxies11010019 10.3847/0004-637X/829/1/55 10.1051/0004-6361/202346228 10.1038/s41550-021-01384-2 10.1093/mnrasl/slaa168 10.1093/mnras/stu1223 10.1086/306742 10.3847/2041-8213/ac8007 10.1088/0004-637X/719/1/722 10.3847/1538-4357/ab2bef 10.1111/j.1365-2966.2011.18477.x 10.1088/0004-637X/730/1/25 10.1093/mnras/stac821 10.1093/mnras/staa2994 10.1086/587832 10.1051/0004-6361/202244418 10.3847/2041-8213/aa991c 10.3847/1538-4357/ab80bd 10.3847/1538-4365/aab5b0 10.3847/2041-8213/ac03b8 10.1086/161749 10.1088/0004-637X/798/2/118 10.3847/2515-5172/ab9088 10.1086/497109 10.3847/2041-8213/ab481c 10.1093/mnras/stab790 10.1103/PhysRevLett.119.161101 10.3847/1538-4357/abb6fd 10.3847/2041-8213/aa9d87 10.3847/2041-8213/aaa401 10.3847/2041-8213/aaad06 10.1046/j.1365-8711.2002.04964.x 10.3847/1538-4357/ac142b 10.1093/mnras/staa983 10.1103/PhysRevD.100.023015 10.1088/0004-637X/787/1/82 10.3847/1538-4357/aca524 10.1073/pnas.20.5.254 10.1093/mnras/stx1533 10.3847/0004-637X/820/1/28 10.1038/nature09466 10.1111/j.1365-2966.2009.15828.x 10.1093/mnras/stac3719 10.1051/0004-6361/202141450 10.1086/526338 10.1038/s41550-022-01874-x 10.1038/s41586-020-03059-w 10.1093/mnras/stab1990 10.1051/0004-6361/202142670 10.1046/j.1365-8711.2003.06392.x 10.1103/PhysRevD.97.021501 10.1038/s41586-020-2439-x 10.1103/PhysRevLett.73.1878 10.1051/0004-6361/201731082 10.1038/s41550-019-0880-2 10.1086/368279 10.1093/mnras/stw483 10.3847/2041-8213/acca83 10.3847/2041-8213/ab960f 10.1086/505742 10.1146/annurev-astro-081915-023322 10.1088/0004-637X/757/1/10 10.1086/421713 10.1093/mnras/stab3722 10.1088/0004-637X/812/2/143 10.1093/mnras/stac379 10.3847/1538-4357/ac7f99 10.1088/0004-637X/728/2/95 10.1088/0004-637X/778/1/66 10.3847/2041-8213/ac0a81 10.1093/mnras/staa066 10.1093/mnras/stx1518 10.1051/0004-6361:20011122 10.3847/1538-4357/acb43f 10.1103/PhysRevD.77.124017 10.1103/PhysRevD.101.063029 10.1007/s11433-020-1593-0 10.1088/0004-637X/711/2/764 10.1093/mnras/staa3466 10.1093/mnras/stz2645 10.1093/mnras/sty1065 10.1051/0004-6361:20054385 10.1093/mnras/stx2195 10.3847/2041-8213/abdfc6 10.1111/j.1365-2966.2012.21124.x 10.1093/mnras/stad3177 10.3847/1538-4357/aafbaa 10.1093/mnras/stw2947 10.1088/1674-4527/20/9/135 10.1051/0004-6361/202244654 10.1088/0004-637X/765/2/158 10.1088/0004-637X/805/2/156 10.3847/1538-4357/aaf37d 10.1038/scientificamerican1068-25 10.3847/2041-8213/abe949 10.3847/1538-4357/ac19b9 10.1051/0004-6361/202038104 10.3847/2041-8213/aad59f 10.1093/mnras/sty2460 10.1086/146780 10.1093/mnras/staa337 10.1103/PhysRevD.102.063006 10.3847/2041-8213/acae99 10.1103/PhysRevLett.32.324 10.1086/523848 10.1088/0004-637X/745/2/109 10.1088/2041-8205/760/2/L36 10.3847/1538-4357/ab7b62 10.3847/1538-4357/ab12e3 10.1088/0004-637X/697/2/1071 10.1086/497420 10.1051/0004-6361/201425191 10.1093/mnras/stv2395 |
ContentType | Journal Article |
Copyright | COPYRIGHT 2023 MDPI AG 2023 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. |
Copyright_xml | – notice: COPYRIGHT 2023 MDPI AG – notice: 2023 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. |
DBID | AAYXX CITATION ABUWG AFKRA AZQEC BENPR BHPHI BKSAR CCPQU DWQXO HCIFZ PCBAR PIMPY PQEST PQQKQ PQUKI PRINS DOA |
DOI | 10.3390/universe10010003 |
DatabaseName | CrossRef ProQuest Central (Alumni) ProQuest Central ProQuest Central Essentials ProQuest Central Natural Science Collection Earth, Atmospheric & Aquatic Science Collection ProQuest One Community College ProQuest Central Korea SciTech Premium Collection Earth, Atmospheric & Aquatic Science Database Publicly Available Content Database ProQuest One Academic Eastern Edition (DO NOT USE) ProQuest One Academic ProQuest One Academic UKI Edition ProQuest Central China DOAJ Directory of Open Access Journals |
DatabaseTitle | CrossRef Publicly Available Content Database ProQuest Central Essentials ProQuest One Academic Eastern Edition Earth, Atmospheric & Aquatic Science Database ProQuest Central (Alumni Edition) SciTech Premium Collection ProQuest One Community College ProQuest Central China Earth, Atmospheric & Aquatic Science Collection ProQuest Central ProQuest One Academic UKI Edition Natural Science Collection ProQuest Central Korea ProQuest One Academic |
DatabaseTitleList | CrossRef Publicly Available Content Database |
Database_xml | – sequence: 1 dbid: DOA name: Directory of Open Access Journals url: https://www.doaj.org/ sourceTypes: Open Website – sequence: 2 dbid: BENPR name: AUTh Library subscriptions: ProQuest Central url: https://www.proquest.com/central sourceTypes: Aggregation Database |
DeliveryMethod | fulltext_linktorsrc |
Discipline | Physics |
EISSN | 2218-1997 |
ExternalDocumentID | oai_doaj_org_article_9ac6e421b50f4b16900c941345a95dc8 A780928249 10_3390_universe10010003 |
GeographicLocations | Brazil |
GeographicLocations_xml | – name: Brazil |
GroupedDBID | 5VS 8FE 8FH AADQD AAYXX ABDBF ADBBV AFKRA AFZYC ALMA_UNASSIGNED_HOLDINGS BCNDV BENPR BHPHI BKSAR CCPQU CITATION GROUPED_DOAJ HCIFZ IAO ITC KQ8 LK5 M7R MODMG M~E OK1 PCBAR PIMPY PROAC ABUWG AZQEC DWQXO PQEST PQQKQ PQUKI PRINS |
ID | FETCH-LOGICAL-c371t-e52274bfc362b1e1040b2b7ba108675582c95a74c9e14b7d9683b840a433974d3 |
IEDL.DBID | DOA |
ISSN | 2218-1997 |
IngestDate | Fri Oct 04 13:13:45 EDT 2024 Thu Oct 10 17:25:22 EDT 2024 Tue Feb 06 05:31:35 EST 2024 Thu Sep 26 17:32:23 EDT 2024 |
IsDoiOpenAccess | true |
IsOpenAccess | true |
IsPeerReviewed | true |
IsScholarly | true |
Issue | 1 |
Language | English |
LinkModel | DirectLink |
MergedId | FETCHMERGED-LOGICAL-c371t-e52274bfc362b1e1040b2b7ba108675582c95a74c9e14b7d9683b840a433974d3 |
ORCID | 0000-0003-4543-0912 0000-0003-3109-9042 0000-0003-1771-1055 0009-0000-3268-9058 0009-0009-4458-8268 0000-0003-4089-3440 |
OpenAccessLink | https://doaj.org/article/9ac6e421b50f4b16900c941345a95dc8 |
PQID | 2918793773 |
PQPubID | 2059542 |
ParticipantIDs | doaj_primary_oai_doaj_org_article_9ac6e421b50f4b16900c941345a95dc8 proquest_journals_2918793773 gale_infotracacademiconefile_A780928249 crossref_primary_10_3390_universe10010003 |
PublicationCentury | 2000 |
PublicationDate | 2024-01-01 |
PublicationDateYYYYMMDD | 2024-01-01 |
PublicationDate_xml | – month: 01 year: 2024 text: 2024-01-01 day: 01 |
PublicationDecade | 2020 |
PublicationPlace | Basel |
PublicationPlace_xml | – name: Basel |
PublicationTitle | Universe (Basel) |
PublicationYear | 2024 |
Publisher | MDPI AG |
Publisher_xml | – name: MDPI AG |
References | Riley (ref_45) 2021; 918 Schwab (ref_15) 2010; 719 Farrow (ref_51) 2019; 876 Ferdman (ref_85) 2014; 443 Falanga (ref_63) 2015; 577 Casares (ref_76) 2002; 329 Breton (ref_49) 2011; 728 Haniewicz (ref_87) 2021; 500 Zhong (ref_29) 2023; 947 Rhoades (ref_7) 1974; 32 Shibata (ref_33) 2019; 100 Kramer (ref_2) 2021; 11 Suwa (ref_23) 2018; 481 Clark (ref_48) 2023; 7 Shamohammadi (ref_106) 2022; 520 ref_126 McKee (ref_119) 2020; 499 Corongiu (ref_94) 2007; 462 Berezina (ref_120) 2017; 470 ref_25 Rezzolla (ref_58) 2018; 852 Freire (ref_123) 2017; 471 Kennedy (ref_73) 2022; 512 Cromartie (ref_14) 2020; 4 Reardon (ref_100) 2016; 455 Istrate (ref_105) 2020; 494 Kandel (ref_75) 2020; 903 Stovall (ref_96) 2018; 854 Valentim (ref_19) 2011; 414 Reardon (ref_98) 2021; 507 Balakrishnan (ref_97) 2023; 942 Margalit (ref_31) 2017; 850 Shao (ref_35) 2020; 101 Atwood (ref_47) 2009; 697 Shahbaz (ref_71) 2017; 472 Berthereau (ref_108) 2023; 674 Desvignes (ref_103) 2016; 458 Corongiu (ref_114) 2023; 671 Knight (ref_68) 2022; 510 Weisberg (ref_80) 2016; 829 Kirichenko (ref_110) 2020; 492 Ridolfi (ref_84) 2019; 409 Sengar (ref_91) 2022; 512 Most (ref_41) 2020; 499 Martinez (ref_82) 2015; 812 Ye (ref_39) 2022; 937 Nomoto (ref_5) 1984; 277 Freire (ref_12) 2008; 675 Jacoby (ref_81) 2006; 644 Demorest (ref_13) 2010; 467 Abbott (ref_30) 2017; 119 Ridolfi (ref_125) 2021; 504 Nice (ref_10) 2005; 634 Casares (ref_66) 2005; 635 Guo (ref_121) 2021; 654 Hiramatsu (ref_17) 2021; 5 ref_86 Martinez (ref_92) 2017; 851 Antoniadis (ref_109) 2012; 423 Zhang (ref_18) 2011; 527 Romani (ref_27) 2022; 934 Swiggum (ref_95) 2015; 805 ref_50 Barr (ref_117) 2017; 465 Ai (ref_60) 2020; 893 Nathanail (ref_37) 2021; 908 ref_55 Fonseca (ref_79) 2014; 787 Zhu (ref_118) 2019; 881 ref_54 ref_52 Burrows (ref_22) 2021; 589 Rawls (ref_69) 2011; 730 Horvath (ref_26) 2020; 63 Kasian (ref_88) 2015; 798 Thorsett (ref_8) 1999; 512 Psaltis (ref_64) 2016; 820 Abbott (ref_36) 2020; 896 Miller (ref_65) 2017; 608 Arzoumanian (ref_115) 2018; 235 Alsing (ref_32) 2018; 478 ref_61 Kandel (ref_24) 2022; 942 Finn (ref_6) 1994; 73 Freire (ref_124) 2003; 340 Farr (ref_53) 2020; 4 Kaplan (ref_78) 2013; 765 Agazie (ref_93) 2021; 922 Hewish (ref_1) 1968; 219 Fonseca (ref_102) 2021; 915 ref_62 Ferdman (ref_89) 2020; 583 Freire (ref_11) 2008; 679 Shao (ref_34) 2020; 102 Serylak (ref_104) 2022; 665 Casares (ref_67) 2010; 401 Wang (ref_28) 2020; 20 Geyer (ref_116) 2023; 674 Romani (ref_57) 2012; 760 Strader (ref_72) 2019; 872 Andersen (ref_111) 2018; 863 Kansabanik (ref_46) 2021; 920 Swiggum (ref_90) 2023; 944 Kiziltan (ref_20) 2013; 778 Bhat (ref_107) 2008; 77 Ferraro (ref_77) 2003; 584 Bhalerao (ref_70) 2012; 757 Ruiz (ref_59) 2018; 97 Ferdman (ref_112) 2010; 711 Martinez (ref_83) 2012; 745 Podsiadlowski (ref_16) 2004; 612 Ai (ref_40) 2023; 526 Abbott (ref_38) 2021; 913 Riley (ref_44) 2019; 887 Cameron (ref_4) 1959; 130 Stovall (ref_122) 2019; 870 Barziv (ref_9) 2001; 377 Ng (ref_113) 2020; 491 Baade (ref_3) 1934; 20 Kandel (ref_74) 2020; 892 Freire (ref_21) 2016; 54 ref_43 ref_42 Voisin (ref_99) 2020; 638 ref_101 Steeghs (ref_56) 2007; 669 |
References_xml | – volume: 527 start-page: A83 year: 2011 ident: ref_18 article-title: Study of measured pulsar masses and their possible conclusions publication-title: Astron. Astrophys. doi: 10.1051/0004-6361/201015532 contributor: fullname: Zhang – ident: ref_62 doi: 10.3390/galaxies11010019 – volume: 829 start-page: 55 year: 2016 ident: ref_80 article-title: Relativistic measurements from timing the binary pulsar PSR B1913+ 16 publication-title: Astrophys. J. doi: 10.3847/0004-637X/829/1/55 contributor: fullname: Weisberg – volume: 674 start-page: A71 year: 2023 ident: ref_108 article-title: Radio timing constraints on the mass of the binary pulsar PSR J1528-3146 publication-title: Astron. Astrophys. doi: 10.1051/0004-6361/202346228 contributor: fullname: Berthereau – volume: 5 start-page: 903 year: 2021 ident: ref_17 article-title: The electron-capture origin of supernova 2018zd publication-title: Nat. Astron. doi: 10.1038/s41550-021-01384-2 contributor: fullname: Hiramatsu – volume: 499 start-page: L82 year: 2020 ident: ref_41 article-title: A lower bound on the maximum mass if the secondary in GW190814 was once a rapidly spinning neutron star publication-title: MNRAS Lett. doi: 10.1093/mnrasl/slaa168 contributor: fullname: Most – volume: 443 start-page: 2183 year: 2014 ident: ref_85 article-title: PSR J1756-2251: A pulsar with a low-mass neutron star companion publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stu1223 contributor: fullname: Ferdman – volume: 512 start-page: 288 year: 1999 ident: ref_8 article-title: Neutron star mass measurements. i. radio pulsars publication-title: Astrophys. J. doi: 10.1086/306742 contributor: fullname: Thorsett – volume: 934 start-page: L18 year: 2022 ident: ref_27 article-title: PSR J0952-0607: The Fastest and Heaviest Known Galactic Neutron Star publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/ac8007 contributor: fullname: Romani – ident: ref_42 – volume: 719 start-page: 722 year: 2010 ident: ref_15 article-title: Further evidence for the bimodal distribution of neutron-star masses publication-title: Astrophys. J. doi: 10.1088/0004-637X/719/1/722 contributor: fullname: Schwab – volume: 881 start-page: 165 year: 2019 ident: ref_118 article-title: Mass measurements for two binary pulsars discovered in the PALFA survey publication-title: Astrophys. J. doi: 10.3847/1538-4357/ab2bef contributor: fullname: Zhu – volume: 414 start-page: 1427 year: 2011 ident: ref_19 article-title: On the mass distribution of neutron stars publication-title: Mon. Not. R. Astron. Soc. doi: 10.1111/j.1365-2966.2011.18477.x contributor: fullname: Valentim – volume: 730 start-page: 25 year: 2011 ident: ref_69 article-title: Refined neutron star mass determinations for six eclipsing x-ray pulsar binaries publication-title: Astrophys. J. doi: 10.1088/0004-637X/730/1/25 contributor: fullname: Rawls – volume: 512 start-page: 57 year: 2022 ident: ref_91 article-title: The High Time Resolution Universe Pulsar Survey—XVII. PSR J1325-6253, a low eccentricity double neutron star system from an ultra-stripped supernova publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stac821 contributor: fullname: Sengar – volume: 499 start-page: 4082 year: 2020 ident: ref_119 article-title: A precise mass measurement of PSR J2045+ 3633 publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/staa2994 contributor: fullname: McKee – volume: 679 start-page: 1433 year: 2008 ident: ref_11 article-title: A massive neutron star in the globular cluster M5 publication-title: Astrophys. J. doi: 10.1086/587832 contributor: fullname: Freire – volume: 671 start-page: A72 year: 2023 ident: ref_114 article-title: PSR J1910–5959 A: A rare gravitational laboratory for testing white dwarf models publication-title: Astron. Astrophys. doi: 10.1051/0004-6361/202244418 contributor: fullname: Corongiu – volume: 850 start-page: L19 year: 2017 ident: ref_31 article-title: Constraining the maximum mass of neutron stars from multi-messenger observations of GW170817 publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/aa991c contributor: fullname: Margalit – volume: 893 start-page: 146 year: 2020 ident: ref_60 article-title: What constraints on the neutron star maximum mass can one pose from GW170817 observations? publication-title: Astrophys. J. doi: 10.3847/1538-4357/ab80bd contributor: fullname: Ai – volume: 235 start-page: 37 year: 2018 ident: ref_115 article-title: The NANOGrav 11-year data set: High-precision timing of 45 millisecond pulsars publication-title: Astrophys. J. Suppl. Ser. doi: 10.3847/1538-4365/aab5b0 contributor: fullname: Arzoumanian – volume: 915 start-page: L12 year: 2021 ident: ref_102 article-title: Refined mass and geometric measurements of the high-mass PSR J0740+ 6620 publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/ac03b8 contributor: fullname: Fonseca – volume: 277 start-page: 791 year: 1984 ident: ref_5 article-title: Evolution of 8–10 solar mass stars toward electron capture supernovae. I-Formation of electron-degenerate O+ NE+ MG cores publication-title: Astrophys. J. doi: 10.1086/161749 contributor: fullname: Nomoto – volume: 798 start-page: 118 year: 2015 ident: ref_88 article-title: The binary companion of young, relativistic pulsar J1906+ 0746 publication-title: Astrophys. J. doi: 10.1088/0004-637X/798/2/118 contributor: fullname: Kasian – volume: 4 start-page: 65 year: 2020 ident: ref_53 article-title: A Population-Informed Mass Estimate for Pulsar J0740+ 6620 publication-title: Res. Notes AAS doi: 10.3847/2515-5172/ab9088 contributor: fullname: Farr – volume: 634 start-page: 1242 year: 2005 ident: ref_10 article-title: A 2.1 M⊙ Pulsar Measured by Relativistic Orbital Decay publication-title: Astrophys. J. doi: 10.1086/497109 contributor: fullname: Nice – volume: 887 start-page: L21 year: 2019 ident: ref_44 article-title: A NICER view of PSR J0030+ 0451: Millisecond pulsar parameter estimation publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/ab481c contributor: fullname: Riley – volume: 504 start-page: 1407 year: 2021 ident: ref_125 article-title: Eight new millisecond pulsars from the first MeerKAT globular cluster census publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stab790 contributor: fullname: Ridolfi – volume: 119 start-page: 161101 year: 2017 ident: ref_30 article-title: GW170817: Observation of gravitational waves from a binary neutron star inspiral publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.119.161101 contributor: fullname: Abbott – volume: 903 start-page: 39 year: 2020 ident: ref_75 article-title: Heated Poles on the Companion of Redback PSR J2339–0533 publication-title: Astrophys. J. doi: 10.3847/1538-4357/abb6fd contributor: fullname: Kandel – volume: 851 start-page: L29 year: 2017 ident: ref_92 article-title: Pulsar J1411+ 2551: A low-mass double neutron star system publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/aa9d87 contributor: fullname: Martinez – volume: 852 start-page: L25 year: 2018 ident: ref_58 article-title: Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/aaa401 contributor: fullname: Rezzolla – volume: 854 start-page: L22 year: 2018 ident: ref_96 article-title: PALFA discovery of a highly relativistic double neutron star binary publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/aaad06 contributor: fullname: Stovall – ident: ref_86 – volume: 329 start-page: 29 year: 2002 ident: ref_76 article-title: VLT spectroscopy of XTE J2123-058 during quiescence: The masses of the two components publication-title: Mon. Not. R. Astron. Soc. doi: 10.1046/j.1365-8711.2002.04964.x contributor: fullname: Casares – volume: 922 start-page: 35 year: 2021 ident: ref_93 article-title: The Green Bank Northern Celestial Cap Pulsar Survey. VI. Discovery and Timing of PSR J1759+ 5036: A Double Neutron Star Binary Pulsar publication-title: Astrophys. J. doi: 10.3847/1538-4357/ac142b contributor: fullname: Agazie – volume: 494 start-page: 4031 year: 2020 ident: ref_105 article-title: PSR J1012+ 5307: A millisecond pulsar with an extremely low-mass white dwarf companion publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/staa983 contributor: fullname: Istrate – volume: 100 start-page: 023015 year: 2019 ident: ref_33 article-title: Constraint on the maximum mass of neutron stars using GW170817 event publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.100.023015 contributor: fullname: Shibata – volume: 787 start-page: 82 year: 2014 ident: ref_79 article-title: A comprehensive study of relativistic gravity using PSR B1534+ 12 publication-title: Astrophys. J. doi: 10.1088/0004-637X/787/1/82 contributor: fullname: Fonseca – volume: 942 start-page: 6 year: 2022 ident: ref_24 article-title: An Optical Study of the Black Widow Population publication-title: Astrophys. J. doi: 10.3847/1538-4357/aca524 contributor: fullname: Kandel – volume: 20 start-page: 254 year: 1934 ident: ref_3 article-title: On super-novae publication-title: Proc. Natl. Acad. Sci. USA doi: 10.1073/pnas.20.5.254 contributor: fullname: Baade – volume: 471 start-page: 857 year: 2017 ident: ref_123 article-title: Long-term observations of the pulsars in 47 Tucanae—II. Proper motions, accelerations and jerks publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stx1533 contributor: fullname: Freire – volume: 820 start-page: 28 year: 2016 ident: ref_64 article-title: The dense matter equation of state from neutron star radius and mass measurements publication-title: Astrophys. J. doi: 10.3847/0004-637X/820/1/28 contributor: fullname: Psaltis – volume: 467 start-page: 1081 year: 2010 ident: ref_13 article-title: A two-solar-mass neutron star measured using Shapiro delay publication-title: Nature doi: 10.1038/nature09466 contributor: fullname: Demorest – volume: 401 start-page: 2517 year: 2010 ident: ref_67 article-title: On the mass of the neutron star in Cyg X-2 publication-title: Mon. Not. R. Astron. Soc. doi: 10.1111/j.1365-2966.2009.15828.x contributor: fullname: Casares – volume: 520 start-page: 1789 year: 2022 ident: ref_106 article-title: Searches for Shapiro delay in seven binary pulsars using the MeerKAT telescope publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stac3719 contributor: fullname: Shamohammadi – volume: 654 start-page: A16 year: 2021 ident: ref_121 article-title: PSR J2222–0137—I. Improved physical parameters for the system publication-title: Astron. Astrophys. doi: 10.1051/0004-6361/202141450 contributor: fullname: Guo – ident: ref_25 – ident: ref_50 – volume: 675 start-page: 670 year: 2008 ident: ref_12 article-title: Eight new millisecond pulsars in NGC 6440 and NGC 6441 publication-title: Astrophys. J. doi: 10.1086/526338 contributor: fullname: Freire – volume: 7 start-page: 451 year: 2023 ident: ref_48 article-title: Neutron star mass estimates from gamma-ray eclipses in spider millisecond pulsar binaries publication-title: Nat. Astron. doi: 10.1038/s41550-022-01874-x contributor: fullname: Clark – volume: 589 start-page: 29 year: 2021 ident: ref_22 article-title: Core-collapse supernova explosion theory publication-title: Nature doi: 10.1038/s41586-020-03059-w contributor: fullname: Burrows – volume: 507 start-page: 2137 year: 2021 ident: ref_98 article-title: The Parkes pulsar timing array second data release: Timing analysis publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stab1990 contributor: fullname: Reardon – volume: 665 start-page: A53 year: 2022 ident: ref_104 article-title: The eccentric millisecond pulsar, PSR J0955-6150—I. Pulse profile analysis, mass measurements, and constraints on binary evolution publication-title: Astron. Astrophys. doi: 10.1051/0004-6361/202142670 contributor: fullname: Serylak – volume: 340 start-page: 1359 year: 2003 ident: ref_124 article-title: Further results from the timing of the millisecond pulsars in 47 Tucanae publication-title: Mon. Not. R. Astron. Soc. doi: 10.1046/j.1365-8711.2003.06392.x contributor: fullname: Freire – ident: ref_126 – ident: ref_101 – volume: 97 start-page: 021501 year: 2018 ident: ref_59 article-title: GW170817, general relativistic magnetohydrodynamic simulations, and the neutron star maximum mass publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.97.021501 contributor: fullname: Ruiz – volume: 583 start-page: 211 year: 2020 ident: ref_89 article-title: Asymmetric mass ratios for bright double neutron-star mergers publication-title: Nature doi: 10.1038/s41586-020-2439-x contributor: fullname: Ferdman – volume: 73 start-page: 1878 year: 1994 ident: ref_6 article-title: Observational constraints on the neutron star mass distribution publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.73.1878 contributor: fullname: Finn – volume: 608 start-page: A31 year: 2017 ident: ref_65 article-title: Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra publication-title: Astron. Astrophys. doi: 10.1051/0004-6361/201731082 contributor: fullname: Miller – volume: 4 start-page: 72 year: 2020 ident: ref_14 article-title: Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar publication-title: Nat. Astron. doi: 10.1038/s41550-019-0880-2 contributor: fullname: Cromartie – volume: 584 start-page: L13 year: 2003 ident: ref_77 article-title: Accurate mass ratio and heating effects in the dual-line millisecond binary pulsar in NGC 6397 publication-title: Astrophys. J. doi: 10.1086/368279 contributor: fullname: Ferraro – volume: 458 start-page: 3341 year: 2016 ident: ref_103 article-title: High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stw483 contributor: fullname: Desvignes – volume: 947 start-page: L21 year: 2023 ident: ref_29 article-title: GRB 211211A: A Neutron Star–White Dwarf Merger? publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/acca83 contributor: fullname: Zhong – volume: 896 start-page: L44 year: 2020 ident: ref_36 article-title: GW190814: Gravitational waves from the coalescence of a 23 solar mass black hole with a 2.6 solar mass compact object publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/ab960f contributor: fullname: Abbott – volume: 644 start-page: L113 year: 2006 ident: ref_81 article-title: Measurement of orbital decay in the double neutron star binary PSR B2127+ 11C publication-title: Astrophys. J. Lett. doi: 10.1086/505742 contributor: fullname: Jacoby – volume: 54 start-page: 401 year: 2016 ident: ref_21 article-title: Masses, radii, and the equation of state of neutron stars publication-title: Annu. Rev. Astron. Astrophys. doi: 10.1146/annurev-astro-081915-023322 contributor: fullname: Freire – ident: ref_55 – volume: 757 start-page: 10 year: 2012 ident: ref_70 article-title: Constraints on the Compact Object Mass in the Eclipsing High-mass X-Ray Binary XMMU J013236. 7+ 303228 in M 33 publication-title: Astrophys. J. doi: 10.1088/0004-637X/757/1/10 contributor: fullname: Bhalerao – volume: 612 start-page: 1044 year: 2004 ident: ref_16 article-title: The effects of binary evolution on the dynamics of core collapse and neutron star kicks publication-title: Astrophys. J. doi: 10.1086/421713 contributor: fullname: Podsiadlowski – volume: 510 start-page: 4736 year: 2022 ident: ref_68 article-title: Eclipse mapping of EXO 0748–676: Evidence for a massive neutron star publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stab3722 contributor: fullname: Knight – volume: 812 start-page: 143 year: 2015 ident: ref_82 article-title: Pulsar J0453+ 1559: A double neutron star system with a large mass asymmetry publication-title: Astrophys. J. doi: 10.1088/0004-637X/812/2/143 contributor: fullname: Martinez – volume: 512 start-page: 3001 year: 2022 ident: ref_73 article-title: Measuring the mass of the black widow PSR J1555-2908 publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stac379 contributor: fullname: Kennedy – volume: 937 start-page: 73 year: 2022 ident: ref_39 article-title: Inferring the Neutron Star Maximum Mass and Lower Mass Gap in Neutron Star–Black Hole Systems with Spin publication-title: Astrophys. J. doi: 10.3847/1538-4357/ac7f99 contributor: fullname: Ye – ident: ref_61 – volume: 728 start-page: 95 year: 2011 ident: ref_49 article-title: Evidence for a Massive Neutron Star from a Radial-velocity Study of the Companion to the Black-widow Pulsar PSR B1957+ 20 publication-title: Astrophys. J. doi: 10.1088/0004-637X/728/2/95 contributor: fullname: Breton – volume: 778 start-page: 66 year: 2013 ident: ref_20 article-title: The neutron star mass distribution publication-title: Astrophys. J. doi: 10.1088/0004-637X/778/1/66 contributor: fullname: Kiziltan – volume: 918 start-page: L27 year: 2021 ident: ref_45 article-title: A NICER view of the massive pulsar PSR J0740+ 6620 informed by radio timing and XMM-Newton spectroscopy publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/ac0a81 contributor: fullname: Riley – volume: 492 start-page: 3032 year: 2020 ident: ref_110 article-title: Searching for optical companions to four binary millisecond pulsars with the Gran Telescopio Canarias publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/staa066 contributor: fullname: Kirichenko – volume: 470 start-page: 4421 year: 2017 ident: ref_120 article-title: The discovery of two mildly recycled binary pulsars in the Northern High Time Resolution Universe pulsar survey publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stx1518 contributor: fullname: Berezina – volume: 377 start-page: 925 year: 2001 ident: ref_9 article-title: The mass of the neutron star in Vela X-1 publication-title: Astron. Astrophys. doi: 10.1051/0004-6361:20011122 contributor: fullname: Barziv – ident: ref_52 – volume: 944 start-page: 154 year: 2023 ident: ref_90 article-title: The Green Bank North Celestial Cap Survey. VII. 12 New Pulsar Timing Solutions publication-title: Astrophys. J. doi: 10.3847/1538-4357/acb43f contributor: fullname: Swiggum – volume: 77 start-page: 124017 year: 2008 ident: ref_107 article-title: Gravitational-radiation losses from the pulsar–white-dwarf binary PSR J1141–6545 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.77.124017 contributor: fullname: Bhat – volume: 101 start-page: 063029 year: 2020 ident: ref_35 article-title: Estimating the maximum gravitational mass of nonrotating neutron stars from the GW170817/GRB 170817A/AT2017gfo observation publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.101.063029 contributor: fullname: Shao – volume: 63 start-page: 129531 year: 2020 ident: ref_26 article-title: Redback/Black Widow Systems as progenitors of the highest neutron star masses and low-mass Black Holes publication-title: Sci. China Phys. Mech. Astron. doi: 10.1007/s11433-020-1593-0 contributor: fullname: Horvath – volume: 711 start-page: 764 year: 2010 ident: ref_112 article-title: A Precise Mass Measurement of the Intermediate-Mass Binary Pulsar PSR J1802–2124 publication-title: Astrophys. J. doi: 10.1088/0004-637X/711/2/764 contributor: fullname: Ferdman – volume: 500 start-page: 4620 year: 2021 ident: ref_87 article-title: Precise mass measurements for the double neutron star system J1829+ 2456 publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/staa3466 contributor: fullname: Haniewicz – volume: 409 start-page: 3860 year: 2019 ident: ref_84 article-title: Upgraded Giant Metrewave Radio Telescope timing of NGC 1851A: A possible millisecond pulsar- neutron star system publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stz2645 contributor: fullname: Ridolfi – volume: 478 start-page: 1377 year: 2018 ident: ref_32 article-title: Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/sty1065 contributor: fullname: Alsing – volume: 462 start-page: 703 year: 2007 ident: ref_94 article-title: The binary pulsar PSR J1811-1736: Evidence of a low amplitude supernova kick publication-title: Astron. Astrophys. doi: 10.1051/0004-6361:20054385 contributor: fullname: Corongiu – volume: 472 start-page: 4287 year: 2017 ident: ref_71 article-title: Properties of the redback millisecond pulsar binary 3FGL J0212. 1+ 5320 publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stx2195 contributor: fullname: Shahbaz – volume: 908 start-page: L28 year: 2021 ident: ref_37 article-title: GW170817 and GW190814: Tension on the Maximum Mass publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/abdfc6 contributor: fullname: Nathanail – volume: 423 start-page: 3316 year: 2012 ident: ref_109 article-title: The relativistic pulsar–white dwarf binary PSR J1738+ 0333—I. Mass determination and evolutionary history publication-title: Mon. Not. R. Astron. Soc. doi: 10.1111/j.1365-2966.2012.21124.x contributor: fullname: Antoniadis – volume: 526 start-page: 6260 year: 2023 ident: ref_40 article-title: What constraints can one pose on the maximum mass of neutron stars from multi-messenger observations? publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stad3177 contributor: fullname: Ai – volume: 872 start-page: 42 year: 2019 ident: ref_72 article-title: Optical spectroscopy and demographics of redback millisecond pulsar binaries publication-title: Astrophys. J. doi: 10.3847/1538-4357/aafbaa contributor: fullname: Strader – volume: 465 start-page: 1711 year: 2017 ident: ref_117 article-title: A massive millisecond pulsar in an eccentric binary publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stw2947 contributor: fullname: Barr – volume: 20 start-page: 135 year: 2020 ident: ref_28 article-title: The formation of neutron star systems through accretion-induced collapse in white-dwarf binaries publication-title: Res. Astron. Astrophys. doi: 10.1088/1674-4527/20/9/135 contributor: fullname: Wang – volume: 674 start-page: A169 year: 2023 ident: ref_116 article-title: Mass measurements and 3D orbital geometry of PSR J1933–6211 publication-title: Astron. Astrophys. doi: 10.1051/0004-6361/202244654 contributor: fullname: Geyer – volume: 765 start-page: 158 year: 2013 ident: ref_78 article-title: A metal-rich low-gravity companion to a massive millisecond pulsar publication-title: Astrophys. J. doi: 10.1088/0004-637X/765/2/158 contributor: fullname: Kaplan – volume: 805 start-page: 156 year: 2015 ident: ref_95 article-title: PSR J1930–1852: A pulsar in the widest known orbit around another neutron star publication-title: Astrophys. J. doi: 10.1088/0004-637X/805/2/156 contributor: fullname: Swiggum – volume: 870 start-page: 74 year: 2019 ident: ref_122 article-title: PSR J2234+ 0611: A new laboratory for Stellar evolution publication-title: Astrophys. J. doi: 10.3847/1538-4357/aaf37d contributor: fullname: Stovall – volume: 219 start-page: 25 year: 1968 ident: ref_1 article-title: Pulsars publication-title: Sci. Am. doi: 10.1038/scientificamerican1068-25 contributor: fullname: Hewish – volume: 913 start-page: L7 year: 2021 ident: ref_38 article-title: Population properties of compact objects from the second LIGO–Virgo gravitational-wave transient catalog publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/abe949 contributor: fullname: Abbott – volume: 920 start-page: 58 year: 2021 ident: ref_46 article-title: Unraveling the eclipse mechanism of a binary millisecond pulsar using broadband radio spectra publication-title: Astrophys. J. doi: 10.3847/1538-4357/ac19b9 contributor: fullname: Kansabanik – volume: 638 start-page: A24 year: 2020 ident: ref_99 article-title: An improved test of the strong equivalence principle with the pulsar in a triple star system publication-title: Astron. Astrophys. doi: 10.1051/0004-6361/202038104 contributor: fullname: Voisin – volume: 863 start-page: L13 year: 2018 ident: ref_111 article-title: A Fourier domain “Jerk” search for binary pulsars publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/aad59f contributor: fullname: Andersen – volume: 481 start-page: 3305 year: 2018 ident: ref_23 article-title: On the minimum mass of neutron stars publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/sty2460 contributor: fullname: Suwa – volume: 130 start-page: 884 year: 1959 ident: ref_4 article-title: Neutron Star Models publication-title: Astrophys. J. doi: 10.1086/146780 contributor: fullname: Cameron – ident: ref_54 – volume: 491 start-page: 1261 year: 2020 ident: ref_113 article-title: A Shapiro delay detection in the pulsar binary system PSR J1811–2405 publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/staa337 contributor: fullname: Ng – volume: 102 start-page: 063006 year: 2020 ident: ref_34 article-title: Maximum mass cutoff in the neutron star mass distribution and the prospect of forming supramassive objects in the double neutron star mergers publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.102.063006 contributor: fullname: Shao – volume: 942 start-page: L35 year: 2023 ident: ref_97 article-title: Missing for 20 yr: MeerKAT Redetects the Elusive Binary Pulsar M30B publication-title: Astrophys. J. Lett. doi: 10.3847/2041-8213/acae99 contributor: fullname: Balakrishnan – volume: 32 start-page: 324 year: 1974 ident: ref_7 article-title: Maximum mass of a neutron star publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.32.324 contributor: fullname: Rhoades – volume: 669 start-page: L85 year: 2007 ident: ref_56 article-title: On the mass of the neutron star in v395 carinae/2s 0921–630 publication-title: Astrophys. J. doi: 10.1086/523848 contributor: fullname: Steeghs – volume: 11 start-page: 041050 year: 2021 ident: ref_2 article-title: Strong-field gravity tests with the double pulsar publication-title: Phys. Rev. X contributor: fullname: Kramer – volume: 745 start-page: 109 year: 2012 ident: ref_83 article-title: The timing of nine globular cluster pulsars publication-title: Astrophys. J. doi: 10.1088/0004-637X/745/2/109 contributor: fullname: Martinez – volume: 760 start-page: L36 year: 2012 ident: ref_57 article-title: PSR J1311-3430: A Heavyweight Neutron Star with a Flyweight Helium Companion publication-title: Astrophys. J. Lett. doi: 10.1088/2041-8205/760/2/L36 contributor: fullname: Romani – volume: 892 start-page: 101 year: 2020 ident: ref_74 article-title: Atmospheric circulation on black widow companions publication-title: Astrophys. J. doi: 10.3847/1538-4357/ab7b62 contributor: fullname: Kandel – ident: ref_43 – volume: 876 start-page: 18 year: 2019 ident: ref_51 article-title: The mass distribution of galactic double neutron stars publication-title: Astrophys. J. doi: 10.3847/1538-4357/ab12e3 contributor: fullname: Farrow – volume: 697 start-page: 1071 year: 2009 ident: ref_47 article-title: The large area telescope on the Fermi gamma-ray space telescope mission publication-title: Astrophys. J. doi: 10.1088/0004-637X/697/2/1071 contributor: fullname: Atwood – volume: 635 start-page: 502 year: 2005 ident: ref_66 article-title: The “k-correction” for irradiated emission lines in lmxbs: Evidence for a massive neutron star in x1822–371 (v691 cra) publication-title: Astrophys. J. doi: 10.1086/497420 contributor: fullname: Casares – volume: 577 start-page: A130 year: 2015 ident: ref_63 article-title: Ephemeris, orbital decay, and masses of ten eclipsing high-mass X-ray binaries publication-title: Astron. Astrophys. doi: 10.1051/0004-6361/201425191 contributor: fullname: Falanga – volume: 455 start-page: 1751 year: 2016 ident: ref_100 article-title: Timing analysis for 20 millisecond pulsars in the Parkes Pulsar Timing Array publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stv2395 contributor: fullname: Reardon |
SSID | ssj0001759978 |
Score | 2.2969642 |
Snippet | Matter at ultra-high densities finds a physical realization inside neutron stars. One key property is their maximum mass, which has far-reaching implications... |
SourceID | doaj proquest gale crossref |
SourceType | Open Website Aggregation Database |
StartPage | 3 |
SubjectTerms | Astronomical research Gravitational waves mass distribution Neutron stars Orbits Pulsars Stars & galaxies Supernovae TOV mass |
SummonAdditionalLinks | – databaseName: ProQuest Central dbid: BENPR link: http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwfV3dSxwxEA9WKfRF1Lb0_Ch5EKQPy-1uks3GFzmtIsKdUnpwfQpJNnsIuqd7d-Cf70w216MFfd0s-zGTzMxvJvkNIceFyY1hXiVCsCKBGeIT62qbeCRr54LXKhCYDkfF9ZjfTMQkJtzmcVvlyiYGQ13NHObI-7nCvthMSnb29Jxg1yisrsYWGh_IVp5xLNNunV-O7n6tsyxSKMBJXX2SAb7vL7v9Dh65hxAQ_OOPAm3_W8Y5eJyrHbIdQ0U66HS7SzZ8s0c-hi2bbv6Z_BlC3Et_IvFt7FlFTVPRoXm5f1w-0jA6q-nILzHbTSGqbOentGMrDiO3rcWOIRRMBJ7KDU8YNNMH_4WMry5_X1wnsVFC4pjMFomHIEpyWzvwRjaDX-Opza20BtsoSSHK3ClhJHfKZ9zKShUls4DsDAeRSF6xr2SzmTX-G6Gu5k4wm_JaQmxlKlV5ACAuky43pSuKHvmxEpd-6vgwNOAIFK3-X7Q9co7y_HsfMlmHC7N2quPC0Mq4wvM8syKtucWiXeoUeFZ4uRKVK3vkBLWhcb0tWuNMPDYAn4vMVXogy1QBbuSqRw5XCtNxIc71etrsvz98QD7lEK902ZVDsrlol_4I4o2F_R4n1SsJYNTG priority: 102 providerName: ProQuest |
Title | Mass Distribution and Maximum Mass of Neutron Stars: Effects of Orbital Inclination Angle |
URI | https://www.proquest.com/docview/2918793773 https://doaj.org/article/9ac6e421b50f4b16900c941345a95dc8 |
Volume | 10 |
hasFullText | 1 |
inHoldings | 1 |
isFullTextHit | |
isPrint | |
link | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwrV1LS8QwEA6iCF7EJ66PJQdBPBTbJmk23nbVZRF2FVHQU0jSVAS3yj7An-9MUkUF8eKp0ISSzuTxfZPkG0IOC5Mbw7xKhGBFAj3EJ9ZVNvEo1s4Fr1QQMB2OisEdv7wX919SfeGZsCgPHA13oowrPM8zK9KKW9zUSZ2CmZcLo0Tp4jXfTHwhUyG6IoUCfhT3JRnw-pN5POfgUXMIicC3dSjI9f82KYeVpr9GVhuISLuxaetkwdcbZDkc1XTTTfIwBLxLz1HwtslVRU1d0qF5exrPxzSUvlR05OcY5aaAJifTUxpVikPJ1cRiphAKUwPexg1f6NaPz36L3PUvbs8GSZMgIXFMZrPEA3iS3FYOViGbwa_x1OZWWoPpk6QQndwpYSR3ymfcylIVHWaB0RkOJpG8ZNtksX6p_Q6hruJOMJvySgKmMqUqPRAPl0mXm44rihY5_jCXfo06GBr4A5pW_zRti_TQnp_1UME6vAC_6sav-i-_tsgRekPjOJtNjDPNdQFoLipW6a7spAr4Ilctsv_hMN0MwKnOFaZRZ1Ky3f9ozR5ZyQHNxNjLPlmcTeb-ANDIzLbJUrd33uvDs3cxur5ph474Dv3c3iI |
link.rule.ids | 315,786,790,870,2115,21416,27955,27956,33777,43838,74657 |
linkProvider | Directory of Open Access Journals |
linkToHtml | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwfV1Nb9QwEB3BVoheEJ9iSwEfkBCHqElsxzEXtKWtFuguCLVSOVm241RIbbbN7kr9-cw4XiqQ4BpH-RjbM--N7TcAbypbWsuDzqTkVYYjJGTOty4LJNYupGh1FDCdzavpqfh8Js9Swm2ZtlVufGJ01M3CU458r9RUF5srxT9cXWdUNYpWV1MJjbuwRZKb9Qi29g_n377fZlmU1MiThvVJjvx-bz3sdwikPUSE4I94FGX7_-WcY8Q5eggPElRkk6FvH8Gd0D2Ge3HLpl8-gR8zxL3sgIRvU80qZruGzezNz8v1JYuti5bNw5qy3QxRZb98zwa14tjytXdUMYShi6BTufEJk-78IjyF06PDk4_TLBVKyDxXxSoLCKKUcK3HaOQK_DWRu9IpZ6mMkpKyLr2WVgmvQyGcanRVc4fMzgo0iRINfwajbtGF58B8K7zkLhetQmxlG90EJCC-UL60ta-qMbzbmMtcDXoYBnkEmdb8bdox7JM9f99HStbxwqI_N2liGG19FURZOJm3wtGiXe41RlZ8uZaNr8fwlnrD0Hxb9dbbdGwAP5eUq8xE1blG3ij0GHY3HWbSRFya22Gz8__m13B_ejI7Nsef5l9ewHaJ2GXItOzCaNWvw0vEHiv3Kg2wXz_g17w |
linkToPdf | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwfV1Lb9QwEB5BKxAXxFNsKeADEuIQbRLbcdwL2tKuymOXClGpnCzbcSokmm2zu1J_fmccL1WR4BpHeYzHM_ONx98AvK1saS0POpOSVxlqSMicb10WiKxdSNHqSGA6m1dHJ-LzqTxN9U_LVFa5sYnRUDcLTznycampLzZXio_bVBZxfDD9cHGZUQcp2mlN7TTuwrYSlUQgtr1_OD_-fpNxUVIjZhr2Kjli_fF6qH0IxENE4OCWb4oU_v8y1NH7TB_BwxQ2sskwz4_hTuiewL1YvumXT-HnDGNgdkAkuKl_FbNdw2b26tf5-pzF0UXL5mFNmW-GEWa_3GMDc3Ec-dY76h7C0FzQCd34hEl39js8g5Pp4Y-PR1lqmpB5ropVFjCgUsK1Hj2TK_DXRO5Kp5yllkpKyrr0WlolvA6FcKrRVc0dojwrUCRKNPw5bHWLLrwA5lvhJXe5aBXGWbbRTUAw4gvlS1v7qhrB-424zMXAjWEQU5Bozd-iHcE-yfPPfcRqHS8s-jOTFonR1ldBlIWTeSscbeDlXqOXxZdr2fh6BO9oNgytvVVvvU1HCPBzicXKTFSda8SQQo9gdzNhJi3KpblRoZ3_D7-B-6hb5uun-ZeX8KDEMGZIuuzC1qpfh1cYhqzc66Rf10CH2_A |
openUrl | ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Mass+Distribution+and+Maximum+Mass+of+Neutron+Stars%3A+Effects+of+Orbital+Inclination+Angle&rft.jtitle=Universe+%28Basel%29&rft.au=L%C3%ADvia+S.+Rocha&rft.au=Jorge+E.+Horvath&rft.au=Lucas+M.+de+S%C3%A1&rft.au=Gustavo+Y.+Chinen&rft.date=2024-01-01&rft.pub=MDPI+AG&rft.eissn=2218-1997&rft.volume=10&rft.issue=1&rft.spage=3&rft_id=info:doi/10.3390%2Funiverse10010003&rft.externalDBID=DOA&rft.externalDocID=oai_doaj_org_article_9ac6e421b50f4b16900c941345a95dc8 |
thumbnail_l | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=2218-1997&client=summon |
thumbnail_m | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=2218-1997&client=summon |
thumbnail_s | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=2218-1997&client=summon |