{ "id": "1101.0414", "version": "v2", "published": "2011-01-02T16:30:54.000Z", "updated": "2011-02-03T14:51:45.000Z", "title": "The Long-term Variability of the X-ray Sources in M82", "authors": [ "Yi-Kuan Chiang", "Albert K. H. Kong" ], "comment": "Accepted for publication in MNRAS", "categories": [ "astro-ph.HE" ], "abstract": "We investigate the long-term variability exhibited by the X-ray point sources in the starburst galaxy M82. By combining 9 Chandra observations taken between 1999 and 2007, we detect 58 X-ray point sources within the D25 isophote of M82 down to a luminosity of ~ 10^37 ergs/s. Of these 58 sources, we identify 3 supernova remnant candidates and one supersoft source. Twenty-six sources in M82 exhibit long-term (i.e., days to years) flux variability and 3 show long-term spectral variability. Furthermore, we classify 26 sources as variables and 10 as persistent sources. Among the total 26 variables, 17 varied by a flux ratio of > 3 and 6 are transient candidates. By comparing with other nearby galaxies, M82 shows extremely strong long-term X-ray variability that 47% of the X-ray sources are variables with a flux ratio of > 3. The strong X-ray variability of M82 suggests that the population is dominated by X-ray binaries.", "revisions": [ { "version": "v2", "updated": "2011-02-03T14:51:45.000Z" } ], "analyses": { "keywords": [ "x-ray sources", "long-term variability", "x-ray point sources", "extremely strong long-term x-ray variability", "flux ratio" ], "tags": [ "journal article" ], "publication": { "doi": "10.1111/j.1365-2966.2011.18466.x", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2011, "month": "Jun", "volume": 414, "number": 2, "pages": 1329 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 883232, "adsabs": "2011MNRAS.414.1329C" } } }