| dc.contributor.author | Arnaboldi, Magda | |
| dc.contributor.author | Bhattacharya, Souradeep | |
| dc.contributor.author | Gerhard, Ortwin | |
| dc.contributor.author | Kobayashi, Chiaki | |
| dc.contributor.author | Freeman, Kenneth C. | |
| dc.contributor.author | Caldwell, Nelson | |
| dc.contributor.author | Hartke, Johanna | |
| dc.contributor.author | McConnachie, Alan | |
| dc.contributor.author | Guhathakurta, Puragra | |
| dc.date.accessioned | 2022-10-21T14:15:03Z | |
| dc.date.available | 2022-10-21T14:15:03Z | |
| dc.date.issued | 2022-10-13 | |
| dc.identifier.citation | Arnaboldi , M , Bhattacharya , S , Gerhard , O , Kobayashi , C , Freeman , K C , Caldwell , N , Hartke , J , McConnachie , A & Guhathakurta , P 2022 , ' The survey of planetary nebulae in Andromeda (M 31) V. Chemical enrichment of the thin and thicker discs of Andromeda. Oxygen to argon abundance ratios for planetary nebulae and H II regions ' , Astronomy & Astrophysics , vol. 666 , A109 . https://doi.org/10.1051/0004-6361/202244258 | |
| dc.identifier.issn | 0004-6361 | |
| dc.identifier.other | ArXiv: http://arxiv.org/abs/2208.02328v1 | |
| dc.identifier.other | ORCID: /0000-0002-4343-0487/work/121257355 | |
| dc.identifier.uri | http://hdl.handle.net/2299/25832 | |
| dc.description | © M. Arnaboldi et al. 2022. This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. | |
| dc.description.abstract | We use oxygen and argon abundances for planetary nebulae (PNe) with low internal extinction (progenitor ages of (>4.5 Gyr) and high extinction (progenitor ages | en |
| dc.format.extent | 14 | |
| dc.format.extent | 1167040 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Astronomy & Astrophysics | |
| dc.subject | astro-ph.GA | |
| dc.title | The survey of planetary nebulae in Andromeda (M 31) V. Chemical enrichment of the thin and thicker discs of Andromeda. Oxygen to argon abundance ratios for planetary nebulae and H II regions | 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 | |
| rioxxterms.versionofrecord | 10.1051/0004-6361/202244258 | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
