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dc.contributor.authorWright, Nick
dc.contributor.authorBarlow, M.J.
dc.contributor.authorGreimel, R.
dc.contributor.authorDrew, J.E.
dc.contributor.authorMatsuura, M.
dc.contributor.authorUnruh, Y.C.
dc.contributor.authorZijlstra, A.A.
dc.date.accessioned2010-06-07T13:30:36Z
dc.date.available2010-06-07T13:30:36Z
dc.date.issued2009
dc.identifier.citationWright , N , Barlow , M J , Greimel , R , Drew , J E , Matsuura , M , Unruh , Y C & Zijlstra , A A 2009 , ' Near-IR spectra of IPHAS extremely red Galactic AGB stars ' , Monthly Notices of the Royal Astronomical Society , vol. 400 , no. 3 , pp. 1413-1426 . https://doi.org/10.1111/j.1365-2966.2009.15536.x
dc.identifier.issn0035-8711
dc.identifier.otherdspace: 2299/4552
dc.identifier.otherORCID: /0000-0003-1192-7082/work/62750071
dc.identifier.urihttp://hdl.handle.net/2299/4552
dc.description‘The definitive version is available at www3.interscience.wiley.com '. Copyright Royal Astronomical Society DOI: 10.1111/j.1365-2966.2009.15536.x
dc.description.abstractWe present a library of 139 near-IR spectra of cool asymptotic giant branch stars that will be useful for comparison with theoretical model atmosphere calculations and for modelling the integrated emission from intermediate-age stellar populations. The source list was selected from the 'extremely red' region of the Isaac Newton Telescope (INT) Photometric Hα Survey (IPHAS) colour–colour plane that is overwhelmingly dominated by very late-type stars. The spectral library also includes a large fraction of S-type and carbon stars. We present a number of spectral classification sequences highlighting the various molecular features identified and discuss a number of rare features with uncertain identifications in the literature. With its focus on particularly cool photospheres, this catalogue serves as a companion to recent spectroscopic atlases of MK standards in the near-IR. Finally, the relationship between IPHAS (r'−i') and (r'− Hα) colours and spectroscopically determined properties is discussed and a strong correlation between the (r'− Hα) colour and the C/O abundance index for S-type and carbon stars is noted. This relation has the potential to separate O-rich, S-type and carbon stars in the Galaxy based on their photometry alone.en
dc.format.extent2249927
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleNear-IR spectra of IPHAS extremely red Galactic AGB starsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1111/j.1365-2966.2009.15536.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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