| dc.contributor.author | Sestito, Federico | |
| dc.contributor.author | Ardern-Arentsen, Anke | |
| dc.contributor.author | Vitali, Sara | |
| dc.contributor.author | Montelius, Martin | |
| dc.contributor.author | Lucchesi, Romain | |
| dc.contributor.author | Venn, Kim A. | |
| dc.contributor.author | Martin, Nicolas F. | |
| dc.contributor.author | Navarro, Julio F. | |
| dc.contributor.author | Starkenburg, Else | |
| dc.date.accessioned | 2024-11-20T09:30:00Z | |
| dc.date.available | 2024-11-20T09:30:00Z | |
| dc.date.issued | 2024-10-22 | |
| dc.identifier.citation | Sestito , F , Ardern-Arentsen , A , Vitali , S , Montelius , M , Lucchesi , R , Venn , K A , Martin , N F , Navarro , J F & Starkenburg , E 2024 , ' The Pristine Inner Galaxy Survey (PIGS) X. Probing the early chemical evolution of the Sagittarius dwarf galaxy with carbon abundances ' , Astronomy & Astrophysics , vol. 690 , no. October 2024 , A333 , pp. 1-16 . https://doi.org/10.1051/0004-6361/202451258 | |
| dc.identifier.issn | 0004-6361 | |
| dc.identifier.other | ArXiv: http://arxiv.org/abs/2406.18636v2 | |
| dc.identifier.uri | http://hdl.handle.net/2299/28473 | |
| dc.description | © 2024 The Author(s). Published by EDP Sciences. This is an open access article distributed under the Creative Commons Attribution License, to view a copy of the license, see: https://creativecommons.org/licenses/by/4.0/ | |
| dc.description.abstract | We aim to constrain the chemo-dynamical properties of the Sagittarius (Sgr) dwarf galaxy using carbon abundances. Our sample from the \textit{Pristine} Inner Galaxy Survey (PIGS) includes $\sim 350$ metal-poor ([Fe/H]~$+0.7$) as in the Galaxy under-predicts the number of CEMP stars in DGs, and for Sgr a cut at [C/Fe]$~\sim +0.35$ may be more appropriate, which brings the frequency of CEMP stars in agreement with that in the Galaxy. | en |
| dc.format.extent | 16 | |
| dc.format.extent | 3338765 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Astronomy & Astrophysics | |
| dc.subject | astro-ph.GA | |
| dc.subject | astro-ph.SR | |
| dc.title | The Pristine Inner Galaxy Survey (PIGS) X. Probing the early chemical evolution of the Sagittarius dwarf galaxy with carbon abundances | en |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.description.status | Peer reviewed | |
| rioxxterms.versionofrecord | 10.1051/0004-6361/202451258 | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
