Star formation in the first galaxies – III. Formation, evolution, and characteristics of the first metal-enriched stellar cluster
We simulate the formation of a low-metallicity (...) stellar cluster at redshift z ~ 14. Beginning with cosmological initial conditions, the simulation utilizes adaptive mesh refinement and sink particles to follow the collapse and evolution of gas past the opacity limit for fragmentation, thus reso...
Saved in:
Published in | Monthly notices of the Royal Astronomical Society Vol. 455; no. 3; p. 3288 |
---|---|
Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
London
Oxford University Press
21.01.2016
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Abstract | We simulate the formation of a low-metallicity (...) stellar cluster at redshift z ~ 14. Beginning with cosmological initial conditions, the simulation utilizes adaptive mesh refinement and sink particles to follow the collapse and evolution of gas past the opacity limit for fragmentation, thus resolving the formation of individual protostellar cores. A time- and location-dependent protostellar radiation field, which heats the gas by absorption on dust, is computed by integration of protostellar evolutionary tracks. The simulation also includes a robust non-equilibrium chemical network that self-consistently treats gas thermodynamics and dust-gas coupling. The system is evolved for 18 kyr after the first protostellar source has formed. In this time span, 30 sink particles representing protostellar cores form with a total mass of 81 M... Their masses range from ~0.1 to 14.4 M... with a median mass ~0.5-1 M... Massive protostars grow by competitive accretion while lower mass protostars are stunted in growth by close encounters and many-body ejections. In the regime explored here, the characteristic mass scale is determined by the cosmic microwave background temperature floor and the onset of efficient dust-gas coupling. It seems unlikely that host galaxies of the first bursts of metal-enriched star formation will be detectable with the James Webb Space Telescope or other next-generation infrared observatories. Instead, the most promising access route to the dawn of cosmic star formation may lie in the scrutiny of metal-poor, ancient stellar populations in the Galactic neighbourhood. The observable targets corresponding to the system simulated here are ultra-faint dwarf satellite galaxies such as Bootes II and Willman I. (ProQuest: ... denotes formulae/symbols omitted.) |
---|---|
AbstractList | We simulate the formation of a low-metallicity (...) stellar cluster at redshift z ~ 14. Beginning with cosmological initial conditions, the simulation utilizes adaptive mesh refinement and sink particles to follow the collapse and evolution of gas past the opacity limit for fragmentation, thus resolving the formation of individual protostellar cores. A time- and location-dependent protostellar radiation field, which heats the gas by absorption on dust, is computed by integration of protostellar evolutionary tracks. The simulation also includes a robust non-equilibrium chemical network that self-consistently treats gas thermodynamics and dust-gas coupling. The system is evolved for 18 kyr after the first protostellar source has formed. In this time span, 30 sink particles representing protostellar cores form with a total mass of 81 M... Their masses range from ~0.1 to 14.4 M... with a median mass ~0.5-1 M... Massive protostars grow by competitive accretion while lower mass protostars are stunted in growth by close encounters and many-body ejections. In the regime explored here, the characteristic mass scale is determined by the cosmic microwave background temperature floor and the onset of efficient dust-gas coupling. It seems unlikely that host galaxies of the first bursts of metal-enriched star formation will be detectable with the James Webb Space Telescope or other next-generation infrared observatories. Instead, the most promising access route to the dawn of cosmic star formation may lie in the scrutiny of metal-poor, ancient stellar populations in the Galactic neighbourhood. The observable targets corresponding to the system simulated here are ultra-faint dwarf satellite galaxies such as Bootes II and Willman I. (ProQuest: ... denotes formulae/symbols omitted.) |
Author | Bromm, Volker Safranek-Shrader, Chalence Milosavljevic, Milo Montgomery, Michael H |
Author_xml | – sequence: 1 givenname: Chalence surname: Safranek-Shrader fullname: Safranek-Shrader, Chalence – sequence: 2 givenname: Michael surname: Montgomery middlename: H fullname: Montgomery, Michael H – sequence: 3 givenname: Milo surname: Milosavljevic fullname: Milosavljevic, Milo – sequence: 4 givenname: Volker surname: Bromm fullname: Bromm, Volker |
BookMark | eNqNkbtKBDEUhoMouF5K-4CNhaO5TLKTUsTLgmCh1kNMTtzITKJJRrQTfATf0Cdx1lUQK6vzFx__OYdvA62GGAChHUoOKFH8sA9J58NcnpioxQqaUC5FxZSUq2hCCBdVM6V0HW3kfE8IqTmTE_R2VXTCLqZeFx8D9gGXOWDnUy74Tnf62UPGH6_veDabHeDTH3Afw1PshmXUwWIz10mbAsnn4k3G0f0q6qHoroKQvJmDxblA141rTTeMMW2hNae7DNvfcxPdnJ5cH59XF5dns-Oji8rUXJZKEMYkWKH0dKoIYURRCsIBCNNQfeuMYtIxIrVRjbZCUKGcscZyK7SyYPkm2lv2PqT4OEAube-zWZwSIA65pdNG0kYJyf6BiobVRFI-ort_0Ps4pDA-sqBqqkTT0JGqlpRJMecErn1IvtfppaWkXdhrv-y13_b4J2mxk0Q |
CitedBy_id | crossref_primary_10_1017_pasa_2016_41 crossref_primary_10_3847_1538_4357_833_1_84 crossref_primary_10_1051_0004_6361_201526356 crossref_primary_10_1093_mnras_stac1549 crossref_primary_10_1093_mnras_stac2479 crossref_primary_10_1093_mnras_stab2497 crossref_primary_10_1093_mnras_stae1027 crossref_primary_10_1093_mnras_stw2120 crossref_primary_10_1093_mnras_stw1307 crossref_primary_10_1093_mnras_sty2984 crossref_primary_10_1093_mnras_staa2144 crossref_primary_10_1093_mnras_stad1201 crossref_primary_10_1093_mnras_staa4017 crossref_primary_10_1093_mnras_sty1217 crossref_primary_10_1093_mnras_stz863 crossref_primary_10_1093_mnras_sty1911 crossref_primary_10_1093_mnras_stw2647 crossref_primary_10_3847_1538_4357_aa8c80 crossref_primary_10_1093_mnras_sty134 crossref_primary_10_1093_mnras_stz2736 crossref_primary_10_1093_mnras_stab2028 crossref_primary_10_1093_mnras_stv2587 crossref_primary_10_1093_mnras_stac2161 crossref_primary_10_3847_1538_4357_acfe08 |
Cites_doi | 10.1046/j.1365-8711.2001.04915.x 10.1086/508679 10.1093/mnras/176.3.483 10.1051/0004-6361:20031279 10.1086/589963 10.1088/0004-637X/737/2/75 10.1088/2041-8205/729/1/L3 10.1088/0004-637X/790/2/128 10.1007/978-94-007-5612-0_3 10.1086/346149 10.1088/0004-637X/723/2/1568 10.1088/0004-637X/727/2/110 10.1146/annurev.astro.44.051905.092549 10.1023/A:1005161325181 10.1016/S0370-1573(01)00019-9 10.1038/nature02071 10.1086/317361 10.1086/305281 10.1086/308776 10.1086/590901 10.1086/155274 10.1093/mnrasl/slu027 10.1088/0004-637X/773/1/19 10.1088/0004-637X/710/2/1343 10.1086/339264 10.1051/0004-6361:20066389 10.1088/0004-637X/691/1/441 10.1086/507978 10.1093/mnras/186.1.59 10.1111/j.1365-2966.2008.14165.x 10.1086/319488 10.1111/j.1365-2966.2008.13326.x 10.1088/0004-637X/721/1/478 10.1111/j.1365-2966.2009.16113.x 10.1086/498015 10.1093/mnras/stu795 10.1038/nature04280 10.1088/0004-637X/735/1/49 10.1111/j.1365-2966.2011.19955.x 10.1086/590417 10.1088/0004-637X/781/2/60 10.1088/0004-637X/731/1/54 10.1093/mnras/176.2.367 10.1086/145971 10.1086/422087 10.1103/RevModPhys.85.809 10.1088/0034-4885/66/10/R03 10.1088/0004-637X/716/1/510 10.1093/mnras/stv982 10.1088/0004-637X/731/1/62 10.1111/j.1365-2966.2006.10391.x 10.1038/nature04011 10.1088/0004-637X/691/1/823 10.1146/annurev.astro.45.071206.100404 10.1111/j.1365-2966.2011.18392.x 10.1111/j.1365-2966.2010.17003.x 10.1038/nature13662 10.1088/0004-637X/703/1/131 10.1111/j.1365-2966.2011.19818.x 10.1126/science.1165857 10.1111/j.1365-2966.2004.08593.x 10.1086/317785 10.1086/431734 10.1088/0004-637X/722/2/1793 10.1046/j.1365-8711.1998.01590.x 10.1086/323947 10.1088/0067-0049/208/1/4 10.1093/mnras/stv492 10.1086/589916 10.1111/j.1365-2966.2012.20731.x 10.1111/j.1365-2966.2012.22078.x 10.1093/mnras/sts011 10.1111/j.1365-2966.2006.11089.x 10.1088/0004-637X/747/1/52 10.1086/518692 10.1086/524187 10.1086/164018 10.1088/0004-637X/761/1/56 10.1093/mnras/stu1532 10.1111/j.1365-2966.2009.15891.x 10.1088/0004-637X/745/1/50 10.1088/0004-637X/692/2/973 10.1088/0067-0049/181/2/321 10.1093/mnras/205.3.705 10.1086/309295 10.1093/mnras/stv565 10.1051/0004-6361:20042178 10.1038/416059a 10.1088/0004-637X/737/2/63 10.1088/0004-637X/796/2/91 10.1086/429955 10.1086/376392 10.1086/520036 10.1111/j.1365-2966.2011.19951.x 10.1088/2041-8205/750/2/L31 10.1111/j.1365-2966.2012.21852.x 10.1093/mnras/277.2.362 10.1051/0004-6361:20010585 10.1088/0004-637X/754/1/71 10.1007/s11214-006-8315-7 10.1086/339393 10.1086/431415 10.1088/0004-637X/693/2/1859 10.1086/341790 10.1093/mnras/stt2307 10.1146/annurev-astro-082708-101642 10.1111/j.1365-2966.2006.10495.x 10.1111/j.1365-2966.2009.15158.x 10.1088/0067-0049/192/1/3 10.1111/j.1365-2966.2011.19538.x 10.1088/0034-4885/76/11/112901 10.1146/annurev.astro.45.051806.110602 10.1111/j.1365-2966.2007.12215.x 10.1111/j.1365-2966.2011.18348.x 10.1088/2041-8205/790/2/L35 10.1086/117064 10.1088/0004-637X/740/2/107 10.1088/0004-637X/743/2/110 10.1086/303547 10.1086/501518 10.1093/mnras/214.3.379 10.1088/0004-637X/738/2/140 10.1146/annurev.astro.42.053102.134057 10.1088/0004-637X/713/1/269 10.1146/annurev-astro-081710-102608 10.1086/510664 10.1046/j.1365-8711.2001.04270.x 10.1088/0004-637X/774/1/64 10.1051/0004-6361:20021525 10.1088/0004-637X/766/2/103 10.1088/0004-637X/759/2/115 10.1086/341256 10.1088/0004-637X/771/1/29 10.1016/j.physrep.2014.02.001 10.1086/588209 10.1088/0004-637X/783/2/75 10.1086/338030 10.1111/j.1365-2966.2006.10214.x 10.1046/j.1365-8711.2001.04311.x 10.1086/379545 10.1111/j.1365-2966.2005.08826.x 10.1111/j.1365-2966.2005.08881.x 10.1088/0004-637X/745/2/154 10.1086/161521 10.1086/500090 10.1093/mnras/stu1980 10.1093/mnras/stv1353 10.1086/375780 10.1088/0004-637X/711/2/1017 |
ContentType | Journal Article |
Copyright | Copyright Oxford University Press, UK Jan 21, 2016 |
Copyright_xml | – notice: Copyright Oxford University Press, UK Jan 21, 2016 |
DBID | AAYXX CITATION 8FD H8D L7M 7TG KL. |
DOI | 10.1093/mnras/stv2545 |
DatabaseName | CrossRef Technology Research Database Aerospace Database Advanced Technologies Database with Aerospace Meteorological & Geoastrophysical Abstracts Meteorological & Geoastrophysical Abstracts - Academic |
DatabaseTitle | CrossRef Technology Research Database Aerospace Database Advanced Technologies Database with Aerospace Meteorological & Geoastrophysical Abstracts - Academic Meteorological & Geoastrophysical Abstracts |
DatabaseTitleList | Meteorological & Geoastrophysical Abstracts - Academic Technology Research Database Technology Research Database |
DeliveryMethod | fulltext_linktorsrc |
Discipline | Meteorology & Climatology Astronomy & Astrophysics |
EISSN | 1365-2966 |
EndPage | 3288 |
ExternalDocumentID | 3913700071 10_1093_mnras_stv2545 |
GroupedDBID | -DZ -~X .2P .I3 0R~ 123 1OC 1TH 29M 4.4 48X 51W 51X 52X 5HH 5LA 5VS 66C 6TJ 702 7PT 8UM AAHTB AAIJN AAJKP AAJQQ AAKDD AAMVS AAOGV AAPQZ AAPXW AARHZ AASNB AAUQX AAVAP AAYXX ABCQN ABCQX ABEML ABEUO ABIXL ABJNI ABNKS ABPEJ ABPTD ABQLI ABXVV ABZBJ ACGFO ACGFS ACGOD ACNCT ACSCC ACUFI ACYRX ACYTK ADEYI ADGZP ADHKW ADHZD ADOCK ADQBN ADRDM ADRIX ADRTK ADVEK ADYVW ADZXQ AECKG AEGPL AEJOX AEKKA AEKSI AEMDU AENEX AENZO AEPUE AETBJ AEWNT AFEBI AFFZL AFIYH AFOFC AFXEN AGINJ AGSYK AHXPO AJEEA AJEUX ALMA_UNASSIGNED_HOLDINGS ALTZX ALUQC APIBT AVWKF AXUDD AZVOD BAYMD BCRHZ BEFXN BEYMZ BFFAM BGNUA BHONS BKEBE BPEOZ BQUQU BTQHN CDBKE CITATION CO8 DAKXR DILTD DR2 DU5 D~K E.L E3Z EBS EE~ EJD ESX F5P F9B FLIZI FLUFQ FOEOM FRJ GAUVT GJXCC H5~ HAR HF~ HW0 HZI HZ~ IHE IX1 J21 JAVBF K48 KBUDW KOP KQ8 KSI KSN L7B LC2 LC3 LP6 LP7 MK4 NGC NMDNZ NOMLY O9- OCL ODMLO OIG OJQWA OK1 P2P P2X P4D PAFKI PEELM PQQKQ Q1. Q11 Q5Y RHF ROX ROZ RUSNO RW1 RX1 RXO TJP TN5 TOX V8K W8V WH7 WRC X5Q X5S YAYTL YKOAZ YXANX 8FD H8D L7M 7TG ABSAR KL. |
ID | FETCH-LOGICAL-c436t-50226ed59a7790020911e5fee5c81abfc926f206ac98ad55159fcdcd3d5a9ded3 |
ISSN | 0035-8711 |
IngestDate | Sun Sep 29 07:20:32 EDT 2024 Fri Aug 16 09:22:57 EDT 2024 Thu Oct 10 17:41:55 EDT 2024 Thu Sep 12 18:44:24 EDT 2024 |
IsDoiOpenAccess | false |
IsOpenAccess | true |
IsPeerReviewed | true |
IsScholarly | true |
Issue | 3 |
Language | English |
LinkModel | OpenURL |
MergedId | FETCHMERGED-LOGICAL-c436t-50226ed59a7790020911e5fee5c81abfc926f206ac98ad55159fcdcd3d5a9ded3 |
Notes | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
OpenAccessLink | https://academic.oup.com/mnras/article-pdf/455/3/3288/9385863/stv2545.pdf |
PQID | 1754195881 |
PQPubID | 42411 |
PageCount | 1 |
ParticipantIDs | proquest_miscellaneous_1786189562 proquest_miscellaneous_1758240613 proquest_journals_1754195881 crossref_primary_10_1093_mnras_stv2545 |
PublicationCentury | 2000 |
PublicationDate | 2016-01-21 |
PublicationDateYYYYMMDD | 2016-01-21 |
PublicationDate_xml | – month: 01 year: 2016 text: 2016-01-21 day: 21 |
PublicationDecade | 2010 |
PublicationPlace | London |
PublicationPlace_xml | – name: London |
PublicationTitle | Monthly notices of the Royal Astronomical Society |
PublicationYear | 2016 |
Publisher | Oxford University Press |
Publisher_xml | – name: Oxford University Press |
References | 2015112717073151000_455.3.3288.3 2015112717073151000_455.3.3288.23 2015112717073151000_455.3.3288.4 2015112717073151000_455.3.3288.24 2015112717073151000_455.3.3288.1 2015112717073151000_455.3.3288.21 2015112717073151000_455.3.3288.2 2015112717073151000_455.3.3288.20 Jeon (2015112717073151000_455.3.3288.67) 2015; 452 2015112717073151000_455.3.3288.7 2015112717073151000_455.3.3288.8 2015112717073151000_455.3.3288.5 2015112717073151000_455.3.3288.6 2015112717073151000_455.3.3288.102 2015112717073151000_455.3.3288.103 2015112717073151000_455.3.3288.100 2015112717073151000_455.3.3288.101 2015112717073151000_455.3.3288.106 2015112717073151000_455.3.3288.107 2015112717073151000_455.3.3288.18 2015112717073151000_455.3.3288.104 2015112717073151000_455.3.3288.19 2015112717073151000_455.3.3288.105 2015112717073151000_455.3.3288.16 2015112717073151000_455.3.3288.17 2015112717073151000_455.3.3288.14 2015112717073151000_455.3.3288.108 2015112717073151000_455.3.3288.109 2015112717073151000_455.3.3288.34 2015112717073151000_455.3.3288.35 2015112717073151000_455.3.3288.32 Cesaroni (2015112717073151000_455.3.3288.31) 2007 2015112717073151000_455.3.3288.33 Greif (2015112717073151000_455.3.3288.53) 2014; 444 2015112717073151000_455.3.3288.30 2015112717073151000_455.3.3288.29 2015112717073151000_455.3.3288.27 2015112717073151000_455.3.3288.28 2015112717073151000_455.3.3288.25 2015112717073151000_455.3.3288.26 2015112717073151000_455.3.3288.45 2015112717073151000_455.3.3288.46 Bovino (2015112717073151000_455.3.3288.22) 2014; 790 2015112717073151000_455.3.3288.43 2015112717073151000_455.3.3288.44 2015112717073151000_455.3.3288.41 2015112717073151000_455.3.3288.42 2015112717073151000_455.3.3288.40 Tan (2015112717073151000_455.3.3288.138) 2014 Walmsley (2015112717073151000_455.3.3288.143) 1995; 1 2015112717073151000_455.3.3288.120 2015112717073151000_455.3.3288.121 2015112717073151000_455.3.3288.124 2015112717073151000_455.3.3288.125 2015112717073151000_455.3.3288.122 2015112717073151000_455.3.3288.123 2015112717073151000_455.3.3288.128 2015112717073151000_455.3.3288.129 2015112717073151000_455.3.3288.126 Beuther (2015112717073151000_455.3.3288.15) 2006; 636 2015112717073151000_455.3.3288.127 2015112717073151000_455.3.3288.38 2015112717073151000_455.3.3288.39 2015112717073151000_455.3.3288.36 2015112717073151000_455.3.3288.37 2015112717073151000_455.3.3288.56 2015112717073151000_455.3.3288.57 2015112717073151000_455.3.3288.54 2015112717073151000_455.3.3288.55 2015112717073151000_455.3.3288.52 2015112717073151000_455.3.3288.50 2015112717073151000_455.3.3288.51 2015112717073151000_455.3.3288.110 2015112717073151000_455.3.3288.113 2015112717073151000_455.3.3288.114 2015112717073151000_455.3.3288.111 2015112717073151000_455.3.3288.112 2015112717073151000_455.3.3288.117 2015112717073151000_455.3.3288.118 2015112717073151000_455.3.3288.115 2015112717073151000_455.3.3288.116 2015112717073151000_455.3.3288.49 2015112717073151000_455.3.3288.47 2015112717073151000_455.3.3288.119 2015112717073151000_455.3.3288.68 2015112717073151000_455.3.3288.65 2015112717073151000_455.3.3288.66 2015112717073151000_455.3.3288.63 2015112717073151000_455.3.3288.64 2015112717073151000_455.3.3288.61 2015112717073151000_455.3.3288.62 2015112717073151000_455.3.3288.60 Bate (2015112717073151000_455.3.3288.9) 2014; 442 2015112717073151000_455.3.3288.142 2015112717073151000_455.3.3288.140 2015112717073151000_455.3.3288.141 2015112717073151000_455.3.3288.147 2015112717073151000_455.3.3288.145 Silk (2015112717073151000_455.3.3288.130) 1983; 205 2015112717073151000_455.3.3288.148 2015112717073151000_455.3.3288.149 2015112717073151000_455.3.3288.58 2015112717073151000_455.3.3288.59 2015112717073151000_455.3.3288.78 2015112717073151000_455.3.3288.79 2015112717073151000_455.3.3288.76 2015112717073151000_455.3.3288.77 2015112717073151000_455.3.3288.74 2015112717073151000_455.3.3288.75 2015112717073151000_455.3.3288.72 2015112717073151000_455.3.3288.73 Bate (2015112717073151000_455.3.3288.11) 1995; 277 2015112717073151000_455.3.3288.70 2015112717073151000_455.3.3288.131 2015112717073151000_455.3.3288.132 2015112717073151000_455.3.3288.135 2015112717073151000_455.3.3288.136 Meece (2015112717073151000_455.3.3288.96) 2014; 783 2015112717073151000_455.3.3288.133 2015112717073151000_455.3.3288.134 2015112717073151000_455.3.3288.139 2015112717073151000_455.3.3288.137 2015112717073151000_455.3.3288.69 2015112717073151000_455.3.3288.89 2015112717073151000_455.3.3288.87 2015112717073151000_455.3.3288.88 2015112717073151000_455.3.3288.85 2015112717073151000_455.3.3288.86 2015112717073151000_455.3.3288.83 2015112717073151000_455.3.3288.84 2015112717073151000_455.3.3288.81 2015112717073151000_455.3.3288.82 2015112717073151000_455.3.3288.80 2015112717073151000_455.3.3288.12 Whitworth (2015112717073151000_455.3.3288.146) 1979; 186 2015112717073151000_455.3.3288.13 2015112717073151000_455.3.3288.10 2015112717073151000_455.3.3288.98 2015112717073151000_455.3.3288.99 2015112717073151000_455.3.3288.97 2015112717073151000_455.3.3288.94 2015112717073151000_455.3.3288.95 2015112717073151000_455.3.3288.92 2015112717073151000_455.3.3288.93 2015112717073151000_455.3.3288.90 Frebel (2015112717073151000_455.3.3288.48) 2013 2015112717073151000_455.3.3288.91 Weiss (2015112717073151000_455.3.3288.144) 2004 2015112717073151000_455.3.3288.150 Kenyon (2015112717073151000_455.3.3288.71) 1994; 108 2015112717073151000_455.3.3288.153 2015112717073151000_455.3.3288.154 2015112717073151000_455.3.3288.151 2015112717073151000_455.3.3288.152 2015112717073151000_455.3.3288.155 |
References_xml | – ident: 2015112717073151000_455.3.3288.26 doi: 10.1046/j.1365-8711.2001.04915.x – ident: 2015112717073151000_455.3.3288.78 doi: 10.1086/508679 – ident: 2015112717073151000_455.3.3288.111 doi: 10.1093/mnras/176.3.483 – ident: 2015112717073151000_455.3.3288.128 doi: 10.1051/0004-6361:20031279 – ident: 2015112717073151000_455.3.3288.40 doi: 10.1086/589963 – ident: 2015112717073151000_455.3.3288.56 doi: 10.1088/0004-637X/737/2/75 – ident: 2015112717073151000_455.3.3288.37 doi: 10.1088/2041-8205/729/1/L3 – ident: 2015112717073151000_455.3.3288.45 doi: 10.1088/0004-637X/790/2/128 – start-page: 55 volume-title: Planets, Stars and Stellar Systems year: 2013 ident: 2015112717073151000_455.3.3288.48 doi: 10.1007/978-94-007-5612-0_3 contributor: fullname: Frebel – ident: 2015112717073151000_455.3.3288.89 doi: 10.1086/346149 – ident: 2015112717073151000_455.3.3288.118 doi: 10.1088/0004-637X/723/2/1568 – ident: 2015112717073151000_455.3.3288.34 doi: 10.1088/0004-637X/727/2/110 – ident: 2015112717073151000_455.3.3288.155 doi: 10.1146/annurev.astro.44.051905.092549 – ident: 2015112717073151000_455.3.3288.57 doi: 10.1023/A:1005161325181 – ident: 2015112717073151000_455.3.3288.5 doi: 10.1016/S0370-1573(01)00019-9 – ident: 2015112717073151000_455.3.3288.24 doi: 10.1038/nature02071 – ident: 2015112717073151000_455.3.3288.49 doi: 10.1086/317361 – ident: 2015112717073151000_455.3.3288.92 doi: 10.1086/305281 – ident: 2015112717073151000_455.3.3288.101 doi: 10.1086/308776 – ident: 2015112717073151000_455.3.3288.114 doi: 10.1086/590901 – ident: 2015112717073151000_455.3.3288.129 doi: 10.1086/155274 – ident: 2015112717073151000_455.3.3288.121 doi: 10.1093/mnrasl/slu027 – ident: 2015112717073151000_455.3.3288.97 doi: 10.1088/0004-637X/773/1/19 – ident: 2015112717073151000_455.3.3288.142 doi: 10.1088/0004-637X/710/2/1343 – ident: 2015112717073151000_455.3.3288.151 doi: 10.1086/339264 – start-page: 149 volume-title: Protostars and Planets VI year: 2014 ident: 2015112717073151000_455.3.3288.138 contributor: fullname: Tan – ident: 2015112717073151000_455.3.3288.2 doi: 10.1051/0004-6361:20066389 – ident: 2015112717073151000_455.3.3288.133 doi: 10.1088/0004-637X/691/1/441 – ident: 2015112717073151000_455.3.3288.152 doi: 10.1086/507978 – volume: 186 start-page: 59 year: 1979 ident: 2015112717073151000_455.3.3288.146 publication-title: MNRAS doi: 10.1093/mnras/186.1.59 contributor: fullname: Whitworth – ident: 2015112717073151000_455.3.3288.7 doi: 10.1111/j.1365-2966.2008.14165.x – ident: 2015112717073151000_455.3.3288.73 doi: 10.1086/319488 – ident: 2015112717073151000_455.3.3288.54 doi: 10.1111/j.1365-2966.2008.13326.x – ident: 2015112717073151000_455.3.3288.63 doi: 10.1088/0004-637X/721/1/478 – ident: 2015112717073151000_455.3.3288.135 doi: 10.1111/j.1365-2966.2009.16113.x – volume: 636 start-page: 323 year: 2006 ident: 2015112717073151000_455.3.3288.15 publication-title: ApJ doi: 10.1086/498015 contributor: fullname: Beuther – volume: 442 start-page: 285 year: 2014 ident: 2015112717073151000_455.3.3288.9 publication-title: MNRAS doi: 10.1093/mnras/stu795 contributor: fullname: Bate – ident: 2015112717073151000_455.3.3288.77 doi: 10.1038/nature04280 – ident: 2015112717073151000_455.3.3288.98 doi: 10.1088/0004-637X/735/1/49 – ident: 2015112717073151000_455.3.3288.8 doi: 10.1111/j.1365-2966.2011.19955.x – ident: 2015112717073151000_455.3.3288.148 doi: 10.1086/590417 – ident: 2015112717073151000_455.3.3288.60 doi: 10.1088/0004-637X/781/2/60 – ident: 2015112717073151000_455.3.3288.106 doi: 10.1088/0004-637X/731/1/54 – ident: 2015112717073151000_455.3.3288.86 doi: 10.1093/mnras/176.2.367 – ident: 2015112717073151000_455.3.3288.122 doi: 10.1086/145971 – start-page: 197 volume-title: Protostars and Planets V year: 2007 ident: 2015112717073151000_455.3.3288.31 contributor: fullname: Cesaroni – ident: 2015112717073151000_455.3.3288.30 doi: 10.1086/422087 – ident: 2015112717073151000_455.3.3288.70 doi: 10.1103/RevModPhys.85.809 – ident: 2015112717073151000_455.3.3288.83 doi: 10.1088/0034-4885/66/10/R03 – ident: 2015112717073151000_455.3.3288.55 doi: 10.1088/0004-637X/716/1/510 – ident: 2015112717073151000_455.3.3288.116 doi: 10.1093/mnras/stv982 – ident: 2015112717073151000_455.3.3288.44 doi: 10.1088/0004-637X/731/1/62 – ident: 2015112717073151000_455.3.3288.126 doi: 10.1111/j.1365-2966.2006.10391.x – ident: 2015112717073151000_455.3.3288.105 doi: 10.1038/nature04011 – ident: 2015112717073151000_455.3.3288.62 doi: 10.1088/0004-637X/691/1/823 – ident: 2015112717073151000_455.3.3288.14 doi: 10.1146/annurev.astro.45.071206.100404 – ident: 2015112717073151000_455.3.3288.36 doi: 10.1111/j.1365-2966.2011.18392.x – ident: 2015112717073151000_455.3.3288.90 doi: 10.1111/j.1365-2966.2010.17003.x – ident: 2015112717073151000_455.3.3288.46 doi: 10.1038/nature13662 – ident: 2015112717073151000_455.3.3288.99 doi: 10.1088/0004-637X/703/1/131 – ident: 2015112717073151000_455.3.3288.127 doi: 10.1111/j.1365-2966.2011.19818.x – ident: 2015112717073151000_455.3.3288.80 doi: 10.1126/science.1165857 – ident: 2015112717073151000_455.3.3288.10 doi: 10.1111/j.1365-2966.2004.08593.x – ident: 2015112717073151000_455.3.3288.94 doi: 10.1086/317785 – ident: 2015112717073151000_455.3.3288.76 doi: 10.1086/431734 – ident: 2015112717073151000_455.3.3288.103 doi: 10.1088/0004-637X/722/2/1793 – ident: 2015112717073151000_455.3.3288.17 doi: 10.1046/j.1365-8711.1998.01590.x – ident: 2015112717073151000_455.3.3288.27 doi: 10.1086/323947 – ident: 2015112717073151000_455.3.3288.28 – ident: 2015112717073151000_455.3.3288.108 doi: 10.1088/0067-0049/208/1/4 – ident: 2015112717073151000_455.3.3288.154 doi: 10.1093/mnras/stv492 – ident: 2015112717073151000_455.3.3288.59 doi: 10.1086/589916 – ident: 2015112717073151000_455.3.3288.61 doi: 10.1111/j.1365-2966.2012.20731.x – ident: 2015112717073151000_455.3.3288.153 doi: 10.1111/j.1365-2966.2012.22078.x – ident: 2015112717073151000_455.3.3288.69 doi: 10.1093/mnras/sts011 – ident: 2015112717073151000_455.3.3288.4 doi: 10.1111/j.1365-2966.2006.11089.x – ident: 2015112717073151000_455.3.3288.39 doi: 10.1088/0004-637X/747/1/52 – ident: 2015112717073151000_455.3.3288.132 doi: 10.1086/518692 – ident: 2015112717073151000_455.3.3288.33 doi: 10.1086/524187 – ident: 2015112717073151000_455.3.3288.136 doi: 10.1086/164018 – ident: 2015112717073151000_455.3.3288.115 doi: 10.1088/0004-637X/761/1/56 – volume: 444 start-page: 1566 year: 2014 ident: 2015112717073151000_455.3.3288.53 publication-title: MNRAS doi: 10.1093/mnras/stu1532 contributor: fullname: Greif – ident: 2015112717073151000_455.3.3288.125 doi: 10.1111/j.1365-2966.2009.15891.x – ident: 2015112717073151000_455.3.3288.150 doi: 10.1088/0004-637X/745/1/50 – ident: 2015112717073151000_455.3.3288.41 doi: 10.1088/0004-637X/692/2/973 – ident: 2015112717073151000_455.3.3288.42 doi: 10.1088/0067-0049/181/2/321 – volume: 205 start-page: 705 year: 1983 ident: 2015112717073151000_455.3.3288.130 publication-title: MNRAS doi: 10.1093/mnras/205.3.705 contributor: fullname: Silk – ident: 2015112717073151000_455.3.3288.1 doi: 10.1086/309295 – ident: 2015112717073151000_455.3.3288.134 doi: 10.1093/mnras/stv565 – ident: 2015112717073151000_455.3.3288.65 doi: 10.1051/0004-6361:20042178 – ident: 2015112717073151000_455.3.3288.88 doi: 10.1038/416059a – ident: 2015112717073151000_455.3.3288.3 doi: 10.1088/0004-637X/737/2/63 – volume-title: Cox and Giuli's Principles of Stellar Structure year: 2004 ident: 2015112717073151000_455.3.3288.144 contributor: fullname: Weiss – ident: 2015112717073151000_455.3.3288.29 doi: 10.1088/0004-637X/796/2/91 – ident: 2015112717073151000_455.3.3288.102 doi: 10.1086/429955 – ident: 2015112717073151000_455.3.3288.32 doi: 10.1086/376392 – ident: 2015112717073151000_455.3.3288.147 doi: 10.1086/520036 – ident: 2015112717073151000_455.3.3288.110 doi: 10.1111/j.1365-2966.2011.19951.x – ident: 2015112717073151000_455.3.3288.117 doi: 10.1088/2041-8205/750/2/L31 – ident: 2015112717073151000_455.3.3288.119 doi: 10.1111/j.1365-2966.2012.21852.x – volume: 277 start-page: 362 year: 1995 ident: 2015112717073151000_455.3.3288.11 publication-title: MNRAS doi: 10.1093/mnras/277.2.362 contributor: fullname: Bate – ident: 2015112717073151000_455.3.3288.13 doi: 10.1051/0004-6361:20010585 – ident: 2015112717073151000_455.3.3288.81 doi: 10.1088/0004-637X/754/1/71 – ident: 2015112717073151000_455.3.3288.50 doi: 10.1007/s11214-006-8315-7 – ident: 2015112717073151000_455.3.3288.100 doi: 10.1086/339393 – ident: 2015112717073151000_455.3.3288.112 doi: 10.1086/431415 – ident: 2015112717073151000_455.3.3288.21 doi: 10.1088/0004-637X/693/2/1859 – ident: 2015112717073151000_455.3.3288.104 doi: 10.1086/341790 – ident: 2015112717073151000_455.3.3288.120 doi: 10.1093/mnras/stt2307 – ident: 2015112717073151000_455.3.3288.6 doi: 10.1146/annurev-astro-082708-101642 – ident: 2015112717073151000_455.3.3288.16 doi: 10.1111/j.1365-2966.2006.10495.x – ident: 2015112717073151000_455.3.3288.68 doi: 10.1111/j.1365-2966.2009.15158.x – ident: 2015112717073151000_455.3.3288.107 doi: 10.1088/0067-0049/192/1/3 – ident: 2015112717073151000_455.3.3288.141 doi: 10.1111/j.1365-2966.2011.19538.x – ident: 2015112717073151000_455.3.3288.23 doi: 10.1088/0034-4885/76/11/112901 – ident: 2015112717073151000_455.3.3288.87 doi: 10.1146/annurev.astro.45.051806.110602 – ident: 2015112717073151000_455.3.3288.139 doi: 10.1111/j.1365-2966.2007.12215.x – ident: 2015112717073151000_455.3.3288.52 doi: 10.1111/j.1365-2966.2011.18348.x – volume: 790 start-page: L35 year: 2014 ident: 2015112717073151000_455.3.3288.22 publication-title: ApJ doi: 10.1088/2041-8205/790/2/L35 contributor: fullname: Bovino – volume: 108 start-page: 251 year: 1994 ident: 2015112717073151000_455.3.3288.71 publication-title: AJ doi: 10.1086/117064 contributor: fullname: Kenyon – ident: 2015112717073151000_455.3.3288.35 doi: 10.1088/0004-637X/740/2/107 – ident: 2015112717073151000_455.3.3288.74 doi: 10.1088/0004-637X/743/2/110 – ident: 2015112717073151000_455.3.3288.131 – ident: 2015112717073151000_455.3.3288.58 doi: 10.1086/303547 – ident: 2015112717073151000_455.3.3288.123 doi: 10.1086/501518 – ident: 2015112717073151000_455.3.3288.82 doi: 10.1093/mnras/214.3.379 – ident: 2015112717073151000_455.3.3288.64 doi: 10.1088/0004-637X/738/2/140 – ident: 2015112717073151000_455.3.3288.12 doi: 10.1146/annurev.astro.42.053102.134057 – ident: 2015112717073151000_455.3.3288.43 doi: 10.1088/0004-637X/713/1/269 – ident: 2015112717073151000_455.3.3288.25 doi: 10.1146/annurev-astro-081710-102608 – ident: 2015112717073151000_455.3.3288.79 doi: 10.1086/510664 – ident: 2015112717073151000_455.3.3288.18 doi: 10.1046/j.1365-8711.2001.04270.x – ident: 2015112717073151000_455.3.3288.145 doi: 10.1088/0004-637X/774/1/64 – ident: 2015112717073151000_455.3.3288.124 doi: 10.1051/0004-6361:20021525 – ident: 2015112717073151000_455.3.3288.38 doi: 10.1088/0004-637X/766/2/103 – ident: 2015112717073151000_455.3.3288.47 doi: 10.1088/0004-637X/759/2/115 – ident: 2015112717073151000_455.3.3288.113 doi: 10.1086/341256 – ident: 2015112717073151000_455.3.3288.51 doi: 10.1088/0004-637X/771/1/29 – ident: 2015112717073151000_455.3.3288.75 doi: 10.1016/j.physrep.2014.02.001 – ident: 2015112717073151000_455.3.3288.149 doi: 10.1086/588209 – volume: 783 start-page: 75 year: 2014 ident: 2015112717073151000_455.3.3288.96 publication-title: ApJ doi: 10.1088/0004-637X/783/2/75 contributor: fullname: Meece – ident: 2015112717073151000_455.3.3288.93 doi: 10.1086/338030 – ident: 2015112717073151000_455.3.3288.20 doi: 10.1111/j.1365-2966.2006.10214.x – ident: 2015112717073151000_455.3.3288.19 doi: 10.1046/j.1365-8711.2001.04311.x – ident: 2015112717073151000_455.3.3288.72 doi: 10.1086/379545 – ident: 2015112717073151000_455.3.3288.95 doi: 10.1111/j.1365-2966.2005.08826.x – ident: 2015112717073151000_455.3.3288.84 doi: 10.1111/j.1365-2966.2005.08881.x – ident: 2015112717073151000_455.3.3288.140 doi: 10.1088/0004-637X/745/2/154 – ident: 2015112717073151000_455.3.3288.137 doi: 10.1086/161521 – ident: 2015112717073151000_455.3.3288.91 doi: 10.1086/500090 – ident: 2015112717073151000_455.3.3288.66 doi: 10.1093/mnras/stu1980 – volume: 452 start-page: 1152 year: 2015 ident: 2015112717073151000_455.3.3288.67 publication-title: MNRAS doi: 10.1093/mnras/stv1353 contributor: fullname: Jeon – ident: 2015112717073151000_455.3.3288.85 doi: 10.1086/375780 – volume: 1 start-page: 137 year: 1995 ident: 2015112717073151000_455.3.3288.143 publication-title: Rev. Mex. Astron. Astrofis. Ser. Conf. contributor: fullname: Walmsley – ident: 2015112717073151000_455.3.3288.109 doi: 10.1088/0004-637X/711/2/1017 |
SSID | ssj0004326 |
Score | 2.4283721 |
Snippet | We simulate the formation of a low-metallicity (...) stellar cluster at redshift z ~ 14. Beginning with cosmological initial conditions, the simulation... |
SourceID | proquest crossref |
SourceType | Aggregation Database |
StartPage | 3288 |
SubjectTerms | Accretion disks Astronomy Computer simulation Cosmology Dwarf stars Formations Galaxies Joining Protostars Star & galaxy formation Star clusters Star formation Stellar evolution |
Title | Star formation in the first galaxies – III. Formation, evolution, and characteristics of the first metal-enriched stellar cluster |
URI | https://www.proquest.com/docview/1754195881 https://search.proquest.com/docview/1758240613 https://search.proquest.com/docview/1786189562 |
Volume | 455 |
hasFullText | 1 |
inHoldings | 1 |
isFullTextHit | |
isPrint | |
link | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwnV1Lb9NAEF6FcuGCSgE1UNAioV5ct4lfsY9VadSgpkiQoNys9T5IqGNXsRNRbvw3fhizLycpCBUulh_r8crzeWZ2PA-E3oLET3gSZq4sPOIGWczcTMTczbJOT2Rd0qGqZ-TwKroYB-8n4aTV-rkRtbSss2P6_Y95Jf_DVTgHfJVZsv_A2YYonIB94C9sgcOwvRePwVJcrNMPbciimIFF54DkJ99gGey4zmAwOHb6dph8qXxl5mWDN-mdus0mckCTmnOw0F2YhAwbZU4lE0_gwTRfVja41_aEKot6mt86RSlj6hoy2kdxWkm3e6nrE5ho0cbBQwQoTX7tfpouCDPJiVOiMqIaTADxL-Wc6x__Jt5_nVwxlD0ZyCr_Cqqe6hF5ueFtmCvkfy7zazNn4-voKl-HTqC28tsPQX4b8cy1yFZxeonu3WJleqBr_xrw-hsS2vd0G0Gj7e3hb5pEV9maFwuZV9ev6hWspMO10rSBAlcf0v748jIdnU9GD9BDr5eEMrD03cd1EbPAV03_mrmbSq_wgBNF_sQQ37aMtg0DZe2MdtFjs0zBpxpzT1CLF3to33LwFh9ita_9YtUeag9h8VUu1D8auHiWzwBs6ugp-iFhihuY4lmBARRYYQtbmGIXS5jiBqZHuAHpEQaI4jsQxaXYILMNUWwgig1En6Fx_3x0duGazh8uDfyodkOwLCPOwoTIcpiwogGVzEPBeUjjLskETbxIeJ2I0CQmLJQ2uaCMMp-FJGGc-c_RTlEWfB9hyjzhcWnnZiwQrJeQju97Au4IBKEd0kaH9q2nN7rAS6oDM_xUsSc17GmjA8uT1MiAKgXjO5DlmuJuG71pLoOElr_d4LMpl2pMrO3mv42Jo26cwGLkxT3GvESP1l_HAdqpF0v-CmzjOnutoPcLDVfGPA |
link.rule.ids | 315,786,790,27955,27956 |
linkProvider | Wiley-Blackwell |
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=Star+formation+in+the+first+galaxies+-+III.+Formation%2C+evolution%2C+and+characteristics+of+the+first+metal-enriched+stellar+cluster&rft.jtitle=Monthly+notices+of+the+Royal+Astronomical+Society&rft.au=Safranek-Shrader%2C+Chalence&rft.au=Montgomery%2C+Michael+H&rft.au=Milosavljevic%2C+Milo&rft.au=Bromm%2C+Volker&rft.date=2016-01-21&rft.issn=0035-8711&rft.eissn=1365-2966&rft.volume=455&rft.issue=3&rft.spage=3288&rft.epage=3288&rft_id=info:doi/10.1093%2Fmnras%2Fstv2545&rft.externalDBID=NO_FULL_TEXT |
thumbnail_l | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=0035-8711&client=summon |
thumbnail_m | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=0035-8711&client=summon |
thumbnail_s | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=0035-8711&client=summon |