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dc.contributor.authorArnaboldi, Magda
dc.contributor.authorBhattacharya, Souradeep
dc.contributor.authorGerhard, Ortwin
dc.contributor.authorKobayashi, Chiaki
dc.contributor.authorFreeman, Kenneth C.
dc.contributor.authorCaldwell, Nelson
dc.contributor.authorHartke, Johanna
dc.contributor.authorMcConnachie, Alan
dc.contributor.authorGuhathakurta, Puragra
dc.date.accessioned2022-10-21T14:15:03Z
dc.date.available2022-10-21T14:15:03Z
dc.date.issued2022-10-13
dc.identifier.citationArnaboldi , 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.issn0004-6361
dc.identifier.otherArXiv: http://arxiv.org/abs/2208.02328v1
dc.identifier.otherORCID: /0000-0002-4343-0487/work/121257355
dc.identifier.urihttp://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.abstractWe use oxygen and argon abundances for planetary nebulae (PNe) with low internal extinction (progenitor ages of (>4.5 Gyr) and high extinction (progenitor agesen
dc.format.extent14
dc.format.extent1167040
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysics
dc.subjectastro-ph.GA
dc.titleThe 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 regionsen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1051/0004-6361/202244258
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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