dc.contributor.author | Yan, Y. T. | |
dc.contributor.author | Henkel, C. | |
dc.contributor.author | Kobayashi, C. | |
dc.contributor.author | Menten, K. M. | |
dc.contributor.author | Gong, Y. | |
dc.contributor.author | Zhang, J. S. | |
dc.contributor.author | Yu, H. Z. | |
dc.contributor.author | Yang, K. | |
dc.contributor.author | Xie, J. J. | |
dc.contributor.author | Wang, X.Y. | |
dc.date.accessioned | 2023-09-18T09:00:05Z | |
dc.date.available | 2023-09-18T09:00:05Z | |
dc.date.issued | 2023-02-14 | |
dc.identifier.citation | Yan , Y T , Henkel , C , Kobayashi , C , Menten , K M , Gong , Y , Zhang , J S , Yu , H Z , Yang , K , Xie , J J & Wang , X Y 2023 , ' Direct measurements of carbon and sulfur isotope ratios in the Milky Way ' , Astronomy & Astrophysics , vol. 670 , A98 , pp. 1/63 . https://doi.org/10.1051/0004-6361/202244584 | |
dc.identifier.issn | 0004-6361 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/2212.03252v1 | |
dc.identifier.other | ORCID: /0000-0002-4343-0487/work/142860197 | |
dc.identifier.uri | http://hdl.handle.net/2299/26678 | |
dc.description | © 2023 The Author(s), published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License (CC BY), https://creativecommons.org/licenses/by/4.0/ | |
dc.description.abstract | Context. Isotope abundance ratios provide a powerful tool for tracing stellar nucleosynthesis, evaluating the composition of stellar ejecta, and constraining the chemical evolution of the Milky Way. Aims. We aim to measure the 12C/13C, 32S/34S, 32S/33S, 32S/36S, 34S/33S, 34S/36S, and 33S/36S isotope ratios across the Milky Way. Methods. With the IRAM 30 meter telescope, we performed observations of the J = 2-1 transitions of CS, C33S, C34S, C36S, 13CS, 13C33S, and 13C34S as well as the J = 3-2 transitions of C33S, C34S, C36S, and 13CS toward a large sample of 110 high-mass star-forming regions. Results. We measured the 12C/13C, 32S/34S, 32S/33S, 32S/36S, 34S/33S, 34S/36S, and 33S/36S abundance ratios with rare isotopologs of CS, thus avoiding significant saturation effects. With accurate distances obtained from parallax data, we confirm previously identified 12C/13C and 32S/34S gradients as a function of galactocentric distance. In the central molecular zone, 12C/13C ratios are higher than suggested by a linear fit to the disk values as a function of galactocentric radius. While 32S/34S ratios near the Galactic center and in the inner disk are similar, this is not the case for 12C/13C, when comparing central values with those near galactocentric radii of 5 kpc. As was already known, there is no 34S/33S gradient but the average ratio of 4.35 ± 0.44 derived from the J = 2-1 transition lines of C34S and C33S is well below previously reported values. A comparison between solar and local interstellar 32S/34S and 34S/33S ratios suggests that the Solar System may have been formed from gas with a particularly high 34S abundance. For the first time, we report positive gradients of 32S/33S, 34S/36S, 33S/36S, and 32S/36S in our Galaxy. The predicted 12C/13C ratios from the latest Galactic chemical-evolution models are in good agreement with our results. While 32S/34S and 32S/36S ratios show larger differences at larger galactocentric distances, 32S/33S ratios show an offset across the entire inner 12 kpc of the Milky Way. | en |
dc.format.extent | 63 | |
dc.format.extent | 16942249 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astronomy & Astrophysics | |
dc.subject | astro-ph.GA | |
dc.subject | nucleosynthesis | |
dc.subject | ISM: molecules | |
dc.subject | abundances | |
dc.subject | ISM: abundances | |
dc.subject | Galaxy: evolution | |
dc.subject | Galaxy: formation | |
dc.subject | HII regions | |
dc.subject | Nuclear reactions | |
dc.subject | Astronomy and Astrophysics | |
dc.subject | Space and Planetary Science | |
dc.title | Direct measurements of carbon and sulfur isotope ratios in the Milky Way | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
dc.identifier.url | http://www.scopus.com/inward/record.url?scp=85148513610&partnerID=8YFLogxK | |
rioxxterms.versionofrecord | 10.1051/0004-6361/202244584 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |