Light curves of six bright soft X-ray transients in M31

dc.contributor.authorNooraee, Nakisa
dc.date.accessioned2017-11-07T09:38:54Z
dc.date.available2017-11-07T09:38:54Z
dc.date.issued2013
dc.description.abstractDisc irradiation is thought to be capable of explaining the global behaviour of the light curves of soft X-ray transients (SXTs). Depending on the strength of the central X-ray emission in irradiating the disc, the light curve may exhibit an exponential or a linear decay. The model predicts that in brighter transients a transition from exponential decline to a linear one may be detectable. In this study, having excluded super-soft sources and hard X-ray transients, a sample of bright SXTs in M31 (L-peak > 10(38) erg s(-1)) has been studied. The expected change in the shape of the decay function is only observed in two of the light curves from the six light curves in the sample. Also, a systematic correlation between the shape of the light curve and the X-ray luminosity has not been seen.en
dc.description.statusPeer revieweden
dc.description.versionPublished Versionen
dc.format.mimetypeapplication/pdfen
dc.identifier.citationNooraee, N. (2013) 'Light curves of six bright soft X-ray transients in M31', Monthly Notices of the Royal Astronomical Society, 428(1), pp. 205-211. doi: 10.1093/mnras/sts024en
dc.identifier.doi10.1093/mnras/sts024
dc.identifier.endpage211
dc.identifier.issn0035-8711
dc.identifier.issued1
dc.identifier.journaltitleMonthly Notices of the Royal Astronomical Societyen
dc.identifier.startpage205
dc.identifier.urihttps://hdl.handle.net/10468/4960
dc.identifier.volume428
dc.language.isoenen
dc.publisherOxford University Pressen
dc.relation.urihttps://academic.oup.com/mnras/article/428/1/205/1048044/Light-curves-of-six-bright-soft-Xray-transients-in
dc.rights© 2012, the Authors. Published by Oxford University Press on behalf of the Royal Astronomical Societyen
dc.subjectBinariesen
dc.subjectCloseen
dc.subjectX-raysen
dc.subjectStarsen
dc.titleLight curves of six bright soft X-ray transients in M31en
dc.typeArticle (peer-reviewed)en
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