Trigonometric Parallaxes of Star-forming Regions beyond the Tangent Point of the Sagittarius Spiral Arm
As part of the BeSSeL Survey, we report trigonometric parallaxes and proper motions of molecular maser sources associated with 13 distant high-mass star-forming regions in the Sagittarius spiral arm of the Milky Way. In particular, we obtain improved parallax distance estimates for three well-studie...
Saved in:
| Published in | The Astrophysical journal Vol. 874; no. 1; pp. 94 - 106 |
|---|---|
| Main Authors | , , , , , , , , , , , |
| Format | Journal Article |
| Language | English |
| Published |
Philadelphia
The American Astronomical Society
20.03.2019
IOP Publishing |
| Subjects | |
| Online Access | Get full text |
Cover
Loading…
| Abstract | As part of the BeSSeL Survey, we report trigonometric parallaxes and proper motions of molecular maser sources associated with 13 distant high-mass star-forming regions in the Sagittarius spiral arm of the Milky Way. In particular, we obtain improved parallax distance estimates for three well-studied regions: for M17, for W51, and for GAL 045.5+00.0. Peculiar motions for all but one source are less than 20 km s−1. We fit a log-periodic spiral to the locations and estimate an average pitch angle of 7 2 1 9. We find that the section of the arm beyond the tangent point in the first quadrant of the Milky Way appears 15 pc below the IAU-defined Galactic plane. |
|---|---|
| AbstractList | As part of the BeSSeL Survey, we report trigonometric parallaxes and proper motions of molecular maser sources associated with 13 distant high-mass star-forming regions in the Sagittarius spiral arm of the Milky Way. In particular, we obtain improved parallax distance estimates for three well-studied regions:
for M17,
for W51, and
for GAL 045.5+00.0. Peculiar motions for all but one source are less than 20 km s
−1
. We fit a log-periodic spiral to the locations and estimate an average pitch angle of 7.°2 ± 1.°9. We find that the section of the arm beyond the tangent point in the first quadrant of the Milky Way appears 15 pc below the IAU-defined Galactic plane. As part of the BeSSeL Survey, we report trigonometric parallaxes and proper motions of molecular maser sources associated with 13 distant high-mass star-forming regions in the Sagittarius spiral arm of the Milky Way. In particular, we obtain improved parallax distance estimates for three well-studied regions: \({1.9}_{-0.1}^{+0.1}\,\mathrm{kpc}\) for M17, \({5.3}_{-0.9}^{+1.3}\,\mathrm{kpc}\) for W51, and \({7.9}_{-0.7}^{+0.9}\,\mathrm{kpc}\) for GAL 045.5+00.0. Peculiar motions for all but one source are less than 20 km s−1. We fit a log-periodic spiral to the locations and estimate an average pitch angle of 7.°2 ± 1.°9. We find that the section of the arm beyond the tangent point in the first quadrant of the Milky Way appears 15 pc below the IAU-defined Galactic plane. As part of the BeSSeL Survey, we report trigonometric parallaxes and proper motions of molecular maser sources associated with 13 distant high-mass star-forming regions in the Sagittarius spiral arm of the Milky Way. In particular, we obtain improved parallax distance estimates for three well-studied regions: for M17, for W51, and for GAL 045.5+00.0. Peculiar motions for all but one source are less than 20 km s−1. We fit a log-periodic spiral to the locations and estimate an average pitch angle of 7 2 1 9. We find that the section of the arm beyond the tangent point in the first quadrant of the Milky Way appears 15 pc below the IAU-defined Galactic plane. |
| Author | Reid, M. J. Dame, T. M. Wu, Y. W. Rygl, K. L. J. Zhang, B. Sakai, N. Xu, Y. Ho, B. Menten, K. M. Zheng, X. W. Brunthaler, A. Li, J. J. |
| Author_xml | – sequence: 1 givenname: Y. W. orcidid: 0000-0003-3188-5983 surname: Wu fullname: Wu, Y. W. organization: National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan – sequence: 2 givenname: M. J. orcidid: 0000-0001-7223-754X surname: Reid fullname: Reid, M. J. organization: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA – sequence: 3 givenname: N. surname: Sakai fullname: Sakai, N. organization: National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan – sequence: 4 givenname: T. M. orcidid: 0000-0003-0109-2392 surname: Dame fullname: Dame, T. M. organization: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA – sequence: 5 givenname: K. M. orcidid: 0000-0001-6459-0669 surname: Menten fullname: Menten, K. M. organization: Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany – sequence: 6 givenname: A. orcidid: 0000-0003-4468-761X surname: Brunthaler fullname: Brunthaler, A. organization: Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany – sequence: 7 givenname: Y. surname: Xu fullname: Xu, Y. organization: Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, People's Republic of China – sequence: 8 givenname: J. J. surname: Li fullname: Li, J. J. organization: Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, People's Republic of China – sequence: 9 givenname: B. orcidid: 0000-0002-3286-5469 surname: Ho fullname: Ho, B. organization: Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, People's Republic of China – sequence: 10 givenname: B. orcidid: 0000-0003-1353-9040 surname: Zhang fullname: Zhang, B. organization: Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, People's Republic of China – sequence: 11 givenname: K. L. J. surname: Rygl fullname: Rygl, K. L. J. organization: Italian ALMA Regional Centre, INAF-Istituto di Radioastronomia, Via P. Gobetti 101, I-40129 Bologna, Italy – sequence: 12 givenname: X. W. surname: Zheng fullname: Zheng, X. W. organization: School of Astronomy and Space Sciences of Nanjing University , Nanjing 210093, People's Republic of China |
| BookMark | eNp9kF1LwzAUhoNMcJveexnw1rq0ydL0cgy_YOBwE7wr-WrNaJOZZOD-vS0VBUFvcsjhfc45PBMwss5qAC5TdIMZyWfpHLOE4Hk-4wKhlJ-A8XdrBMYIIZJQnL-egUkIu_6bFcUY1Ftvamddq6M3Eq65503DP3SAroKbyH1SOd8aW8NnXRtnAxT66KyC8U3DLbe1thGuneneDuibG16b2IHmEOBmb7p5cOHbc3Ba8Sboi686BS93t9vlQ7J6un9cLlaJxDmJCaGMZJVkNFNC4EoQrhSt0kJgRSqWUiGkQprSVDBN80IwlSPJMUIZyZTMOJ6Cq2Hu3rv3gw6x3LmDt93KMsN0znCK86JLoSElvQvB66rce9NyfyxTVPY6y95d2bsrB50dQn8h0kQeOyXRc9P8B14PoHH7n2P-jH8C_ZKK_A |
| CitedBy_id | crossref_primary_10_1007_s10509_024_04298_3 crossref_primary_10_1093_mnras_stac346 crossref_primary_10_1093_mnras_stz2199 crossref_primary_10_1016_j_newast_2022_101896 crossref_primary_10_1088_1674_4527_20_10_159 crossref_primary_10_1007_s10509_019_3639_4 crossref_primary_10_3847_2041_8213_ab5309 crossref_primary_10_1093_mnras_stae987 crossref_primary_10_1007_s00159_020_00126_z crossref_primary_10_1051_0004_6361_202450530 crossref_primary_10_1017_pasa_2024_61 crossref_primary_10_3847_1538_4357_ab700a crossref_primary_10_3847_1538_4357_ab4a11 crossref_primary_10_3847_1538_4357_ab12e0 crossref_primary_10_1093_pasj_psaa026 crossref_primary_10_1088_1538_3873_aba840 crossref_primary_10_3847_1538_4365_abd8cf crossref_primary_10_3847_1538_4365_ac634c crossref_primary_10_1093_mnras_staa357 crossref_primary_10_1017_pasa_2022_20 crossref_primary_10_3847_1538_3881_ad4030 crossref_primary_10_3847_1538_4357_ac2151 crossref_primary_10_1051_0004_6361_202040073 crossref_primary_10_3390_universe8080390 crossref_primary_10_1051_0004_6361_202039768 crossref_primary_10_1093_pasj_psaa018 crossref_primary_10_3847_1538_3881_ac3d90 crossref_primary_10_1093_mnras_stab2704 crossref_primary_10_3847_1538_3881_ad9002 |
| Cites_doi | 10.1093/pasj/63.3.513 10.1088/0004-637X/693/1/419 10.1088/0004-637X/783/2/130 10.1093/pasj/psv045 10.1093/pasj/psu106 10.1093/pasj/62.1.101 10.1086/500091 10.1051/0004-6361/201322765 10.1093/pasj/62.2.287 10.1088/0004-637X/733/1/25 10.1086/184412 10.1093/mnras/121.2.123 10.1134/S1063773716030026 10.1088/0004-637X/700/1/137 10.3847/0004-637X/823/2/77 10.1088/0004-637X/720/2/1055 10.1126/sciadv.1600878 10.3847/1538-3881/aa7850 10.1088/0004-637X/800/1/53 10.1086/318388 10.1093/mnras/stw1019 10.1093/mnras/278.1.27 10.1086/174988 10.1093/pasj/psu129 10.1093/mnras/stv847 10.1086/513572 10.1088/0004-637X/693/1/413 10.1088/0004-637X/693/1/397 10.1051/0004-6361/200811568 10.1093/mnras/stx729 |
| ContentType | Journal Article |
| Copyright | 2019. The American Astronomical Society. All rights reserved. Copyright IOP Publishing Mar 20, 2019 |
| Copyright_xml | – notice: 2019. The American Astronomical Society. All rights reserved. – notice: Copyright IOP Publishing Mar 20, 2019 |
| DBID | AAYXX CITATION 7TG 8FD H8D KL. L7M |
| DOI | 10.3847/1538-4357/ab001a |
| DatabaseName | CrossRef Meteorological & Geoastrophysical Abstracts Technology Research Database Aerospace Database Meteorological & Geoastrophysical Abstracts - Academic Advanced Technologies Database with Aerospace |
| DatabaseTitle | CrossRef Aerospace Database Meteorological & Geoastrophysical Abstracts Technology Research Database Advanced Technologies Database with Aerospace Meteorological & Geoastrophysical Abstracts - Academic |
| DatabaseTitleList | CrossRef Aerospace Database |
| DeliveryMethod | fulltext_linktorsrc |
| Discipline | Astronomy & Astrophysics Physics |
| DocumentTitleAlternate | Trigonometric Parallaxes of Star-forming Regions beyond the Tangent Point of the Sagittarius Spiral Arm |
| EISSN | 1538-4357 |
| ExternalDocumentID | 10_3847_1538_4357_ab001a apjab001a |
| GrantInformation_xml | – fundername: Chinese NSF grantid: 11673051 – fundername: Chinese NSF grantid: 11673066 – fundername: Italian Ministero dell'Istruzione Universita e Ricerca grantid: CUP C52I13000140001 – fundername: Foundation of the Chinese Academy of Sciences grantid: XAB2016A06 – fundername: Chinese NSF grantid: 11873019 |
| GroupedDBID | -DZ -~X 123 1JI 23N 2FS 2WC 4.4 6J9 85S AAFWJ AAGCD AAJIO ABHWH ACBEA ACGFS ACHIP ACNCT ADACN AEFHF AENEX AFPKN AKPSB ALMA_UNASSIGNED_HOLDINGS ASPBG ATQHT AVWKF AZFZN CJUJL CRLBU CS3 EBS EJD F5P FRP GROUPED_DOAJ IJHAN IOP KOT M~E N5L O3W O43 OK1 PJBAE RIN RNS ROL SJN SY9 T37 TN5 TR2 WH7 XSW AAYXX CITATION 7TG 8FD AEINN H8D KL. L7M |
| ID | FETCH-LOGICAL-c374t-46842fc862dbb3fb4add6f19b3d4f816bbcd0e661b8e679b8d70ca300242dc2a3 |
| IEDL.DBID | O3W |
| ISSN | 0004-637X |
| IngestDate | Wed Aug 13 11:20:42 EDT 2025 Tue Jul 01 04:09:47 EDT 2025 Thu Apr 24 22:59:13 EDT 2025 Wed Aug 21 03:33:05 EDT 2024 |
| IsPeerReviewed | true |
| IsScholarly | true |
| Issue | 1 |
| Language | English |
| LinkModel | DirectLink |
| MergedId | FETCHMERGED-LOGICAL-c374t-46842fc862dbb3fb4add6f19b3d4f816bbcd0e661b8e679b8d70ca300242dc2a3 |
| Notes | AAS12833 Stars and Stellar Physics ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
| ORCID | 0000-0001-7223-754X 0000-0003-4468-761X 0000-0002-3286-5469 0000-0003-0109-2392 0000-0003-1353-9040 0000-0003-3188-5983 0000-0001-6459-0669 |
| PQID | 2365831379 |
| PQPubID | 4562441 |
| PageCount | 13 |
| ParticipantIDs | crossref_citationtrail_10_3847_1538_4357_ab001a proquest_journals_2365831379 iop_journals_10_3847_1538_4357_ab001a crossref_primary_10_3847_1538_4357_ab001a |
| ProviderPackageCode | CITATION AAYXX |
| PublicationCentury | 2000 |
| PublicationDate | 2019-03-20 |
| PublicationDateYYYYMMDD | 2019-03-20 |
| PublicationDate_xml | – month: 03 year: 2019 text: 2019-03-20 day: 20 |
| PublicationDecade | 2010 |
| PublicationPlace | Philadelphia |
| PublicationPlace_xml | – name: Philadelphia |
| PublicationTitle | The Astrophysical journal |
| PublicationTitleAbbrev | APJ |
| PublicationTitleAlternate | Astrophys. J |
| PublicationYear | 2019 |
| Publisher | The American Astronomical Society IOP Publishing |
| Publisher_xml | – name: The American Astronomical Society – name: IOP Publishing |
| References | Honma (apjab001abib9) 2015; 67 Breen (apjab001abib3) 2015; 450 Sato (apjab001abib23) 2010a; 62 Reid (apjab001abib17) 2017; 154 Chibueze (apjab001abib4) 2016; 460 Zhang (apjab001abib31) 2009; 693 Reid (apjab001abib20) 2009a; 693 Reid (apjab001abib22) 2009b; 700 Nagayama (apjab001abib14) 2015; 67 Oh (apjab001abib15) 2010; 62 Reid (apjab001abib18) 2016; 823 Kurayama (apjab001abib12) 2011; 63 Malhotra (apjab001abib13) 1994; 437 Wu (apjab001abib26) 2014; 566 Bobylev (apjab001abib2) 2016; 42 Blaauw (apjab001abib1) 1960; 121 Sato (apjab001abib24) 2010b; 720 Schuller (apjab001abib25) 2009; 504 Chibueze (apjab001abib5) 2014; 66 Deller (apjab001abib7) 2007; 119 Persic (apjab001abib16) 1996; 281 Dame (apjab001abib6) 2001; 547 Jackson (apjab001abib11) 2006; 163 Yao (apjab001abib30) 2017; 468 Reid (apjab001abib21) 2014; 783 Xu (apjab001abib28) 2016; 2 Honig (apjab001abib8) 2015; 800 Xu (apjab001abib27) 2011; 733 Reid (apjab001abib19) 1985; 288 Xu (apjab001abib29) 2009; 693 |
| References_xml | – volume: 63 start-page: 513 year: 2011 ident: apjab001abib12 publication-title: PASJ doi: 10.1093/pasj/63.3.513 – volume: 693 start-page: 419 year: 2009 ident: apjab001abib31 publication-title: ApJ doi: 10.1088/0004-637X/693/1/419 – volume: 783 start-page: 130 year: 2014 ident: apjab001abib21 publication-title: ApJ doi: 10.1088/0004-637X/783/2/130 – volume: 67 start-page: 70 year: 2015 ident: apjab001abib9 publication-title: PASJ doi: 10.1093/pasj/psv045 – volume: 66 start-page: 104 year: 2014 ident: apjab001abib5 publication-title: PASJ doi: 10.1093/pasj/psu106 – volume: 62 start-page: 101 year: 2010 ident: apjab001abib15 publication-title: PASJ doi: 10.1093/pasj/62.1.101 – volume: 163 start-page: 145 year: 2006 ident: apjab001abib11 publication-title: ApJS doi: 10.1086/500091 – volume: 566 start-page: A17 year: 2014 ident: apjab001abib26 publication-title: A&A doi: 10.1051/0004-6361/201322765 – volume: 62 start-page: 287 year: 2010a ident: apjab001abib23 publication-title: PASJ doi: 10.1093/pasj/62.2.287 – volume: 733 start-page: 25 year: 2011 ident: apjab001abib27 publication-title: ApJ doi: 10.1088/0004-637X/733/1/25 – volume: 288 start-page: 17 year: 1985 ident: apjab001abib19 publication-title: ApJ doi: 10.1086/184412 – volume: 121 start-page: 123 year: 1960 ident: apjab001abib1 publication-title: MNRAS doi: 10.1093/mnras/121.2.123 – volume: 42 start-page: 182 year: 2016 ident: apjab001abib2 publication-title: AstL doi: 10.1134/S1063773716030026 – volume: 700 start-page: 137 year: 2009b ident: apjab001abib22 publication-title: ApJ doi: 10.1088/0004-637X/700/1/137 – volume: 823 start-page: 77 year: 2016 ident: apjab001abib18 publication-title: ApJ doi: 10.3847/0004-637X/823/2/77 – volume: 720 start-page: 1055 year: 2010b ident: apjab001abib24 publication-title: ApJ doi: 10.1088/0004-637X/720/2/1055 – volume: 2 year: 2016 ident: apjab001abib28 publication-title: SciA doi: 10.1126/sciadv.1600878 – volume: 154 start-page: 63 year: 2017 ident: apjab001abib17 publication-title: AJ doi: 10.3847/1538-3881/aa7850 – volume: 800 start-page: 53 year: 2015 ident: apjab001abib8 publication-title: ApJ doi: 10.1088/0004-637X/800/1/53 – volume: 547 start-page: 792 year: 2001 ident: apjab001abib6 publication-title: ApJ doi: 10.1086/318388 – volume: 460 start-page: 1839 year: 2016 ident: apjab001abib4 publication-title: MNRAS doi: 10.1093/mnras/stw1019 – volume: 281 start-page: 27 year: 1996 ident: apjab001abib16 publication-title: MNRAS doi: 10.1093/mnras/278.1.27 – volume: 437 start-page: 194 year: 1994 ident: apjab001abib13 publication-title: ApJ doi: 10.1086/174988 – volume: 67 start-page: 65 year: 2015 ident: apjab001abib14 publication-title: PASJ doi: 10.1093/pasj/psu129 – volume: 450 start-page: 4109 year: 2015 ident: apjab001abib3 publication-title: MNRAS doi: 10.1093/mnras/stv847 – volume: 119 start-page: 318 year: 2007 ident: apjab001abib7 publication-title: PASP doi: 10.1086/513572 – volume: 693 start-page: 413 year: 2009 ident: apjab001abib29 publication-title: ApJ doi: 10.1088/0004-637X/693/1/413 – volume: 693 start-page: 397 year: 2009a ident: apjab001abib20 publication-title: ApJ doi: 10.1088/0004-637X/693/1/397 – volume: 504 start-page: 415 year: 2009 ident: apjab001abib25 publication-title: A&A doi: 10.1051/0004-6361/200811568 – volume: 468 start-page: 3289 year: 2017 ident: apjab001abib30 publication-title: MNRAS doi: 10.1093/mnras/stx729 |
| SSID | ssj0004299 |
| Score | 2.4943562 |
| Snippet | As part of the BeSSeL Survey, we report trigonometric parallaxes and proper motions of molecular maser sources associated with 13 distant high-mass... |
| SourceID | proquest crossref iop |
| SourceType | Aggregation Database Enrichment Source Index Database Publisher |
| StartPage | 94 |
| SubjectTerms | astrometry Astrophysics Galaxy: kinematics and dynamics Galaxy: structure masers Massive stars Milky Way Parallax Pitch (inclination) Star formation Stars & galaxies stars: formation |
| Title | Trigonometric Parallaxes of Star-forming Regions beyond the Tangent Point of the Sagittarius Spiral Arm |
| URI | https://iopscience.iop.org/article/10.3847/1538-4357/ab001a https://www.proquest.com/docview/2365831379 |
| Volume | 874 |
| hasFullText | 1 |
| inHoldings | 1 |
| isFullTextHit | |
| isPrint | |
| link | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwjV1RS8MwEA5zIvgiOhWnc-RBBR_q2iZLWnwSUdQHN3Ti3kqSpmPgVlkn6L_3rukmoogvJZRLGnLNfd8luQshR1qFKbMq9HwjDTgogfF0LAJPca4QQAE2ygOy9-Lmid8Nu8MaOV_GwuSvlek_g6JLFOyGEOc3A1vaKecooLzsKIR8IEerLBIRel499vwVFBnGFfflnmBy6PYof23hGyatwHd_GOYSba43yUZFE-mF69QWqdlpg-xdFLhwnU8-6Akty25domiQtb4rbZPRAPxtFMKrsgztqxkulb_bguYZBWo585CmAmDRB4tnkQuqyyAWCkyQDlQZakX7-RieUAFfPqrReA4Vx28FfcR9eezXZIc8XV8NLm-86jYFzzDJ5x7HHbfMgAeTas0yzcGyiSyINUt5FgVCa5P6FuBaR1bIWEep9I1iJYinJlRsl9Sn-dTuERoHOu0azJ3ncy4tUJ5uoP1MagHuSRSqJuksxjMxVapxvPHiJQGXAzWQoAYS1EDiNNAkp8sary7Nxh-yx6CipJprxR9yrYUSv4RDBpSLBUzG-_9s5oCsA0mK8dxZ6LdIfT57s4dAROa6TVZue_12-dt9AiDa1o0 |
| linkProvider | IOP Publishing |
| linkToPdf | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwjV3dS8MwEA86UXwRP9n8zIMKPtS1TZasj6IOv9DhJu6tJGk6Bm4d6wT9771Lq0MU8aWEcklDrrnf7_JxR8ihVmHCrAo930gDDkpgPB2JwFOcKwRQgA13QPZeXD3xm16jV-Y5dXdhsnFp-k-hWAQKLoYQ5zcDW1p3cxRQXtYVQr6qj5N0niw0mBCYu-GBPc8uRoZRyX-5J5jsFfuUv7byDZfm4ds_jLNDnNYqWSmpIj0rOrZG5uxonVTPcly8zobv9Ji6crE2ka-TxXZR2iD9LvjcKITpsgxtqwkul7_ZnGYpBXo58ZCqAmjRR4vnkXOq3UUWCmyQdpW7bkXb2QCeUAFfdlR_MIWKg9ecdnBvHvs13CRPrcvu-ZVXZlTwDJN86nHcdUsNeDGJ1izVHKybSINIs4SnzUBobRLfAmTrphUy0s1E-kYxB-SJCRXbIpVRNrJVQqNAJw2D8fN8zqUF2tMItJ9KLcBFaYaqRuqf4xmbMtw4Zr14icHtQA3EqIEYNRAXGqiRk68a4yLUxh-yR6CiuJxv-R9yu59KnAmHDGgXC5iMtv_ZzAFZal-04rvr-9sdsgycKcJjaKG_SyrTyavdA14y1fvu3_sAYmnZcw |
| 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=Trigonometric+Parallaxes+of+Star-forming+Regions+beyond+the+Tangent+Point+of+the+Sagittarius+Spiral+Arm&rft.jtitle=The+Astrophysical+journal&rft.au=Wu%2C+Y+W&rft.au=Reid%2C+M+J&rft.au=Sakai%2C+N&rft.au=Dame%2C+T+M&rft.date=2019-03-20&rft.pub=IOP+Publishing&rft.issn=0004-637X&rft.eissn=1538-4357&rft.volume=874&rft.issue=1&rft_id=info:doi/10.3847%2F1538-4357%2Fab001a&rft.externalDBID=NO_FULL_TEXT |
| thumbnail_l | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=0004-637X&client=summon |
| thumbnail_m | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=0004-637X&client=summon |
| thumbnail_s | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=0004-637X&client=summon |