{ "id": "1210.3695", "version": "v1", "published": "2012-10-13T10:53:40.000Z", "updated": "2012-10-13T10:53:40.000Z", "title": "The Local Group Galaxy NGC 6822 and its Asymptotic Giant Branch Stars", "authors": [ "Patricia A. Whitelock", "John W. Menzies", "Michael W. Feast", "Francois Nsengiyumva", "Noriyuki Matsunaga" ], "comment": "MNRAS in press", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "JHKs photometry is presented from a 3.5 year survey of the central regions of the irregular galaxy NGC6822. The morphology of the colour-magnitude and colour-colour diagrams is discussed with particular reference to M, S and C-type AGB stars and to M-supergiants. Mean JHKs magnitudes and periods are given for 11 O-rich and 50 presumed C-rich Miras. Data are also listed for 27 large amplitude AGB stars without periods and for 69 small amplitude AGB variables. The slope of the bolometric period-luminosity relation for the C-rich Miras is in good agreement with that in the LMC. Distance moduli derived from the C- and O-rich Miras are in agreement with other estimates. The period distribution of C-rich Miras in NGC6822 is similar to that in the Magellanic Clouds, but differs from that in the dwarf spheroidals in the Local Group. In the latter there is a significant proportion of large amplitude, short period variables indicating a population producing old carbon-rich AGB stars.", "revisions": [ { "version": "v1", "updated": "2012-10-13T10:53:40.000Z" } ], "analyses": { "keywords": [ "asymptotic giant branch stars", "local group galaxy ngc", "old carbon-rich agb stars", "producing old carbon-rich agb", "c-rich miras" ], "tags": [ "journal article" ], "publication": { "doi": "10.1093/mnras/sts188", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2013, "month": "Jan", "volume": 428, "number": 3, "pages": 2216 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1190583, "adsabs": "2013MNRAS.428.2216W" } } }