X-ray and optical studies of soft x-ray transients in M31

Show simple item record

dc.contributor.advisor Callanan, Paul en
dc.contributor.author Nooraee, Nakisa
dc.date.accessioned 2014-04-09T15:37:11Z
dc.date.available 2014-04-09T15:37:11Z
dc.date.issued 2014
dc.date.submitted 2014
dc.identifier.citation Nooraee, N. 2014. X-ray and optical studies of soft x-ray transients in M31. PhD Thesis, University College Cork. en
dc.identifier.endpage 121
dc.identifier.uri http://hdl.handle.net/10468/1514
dc.description.abstract Soft X-ray transients (SXTs) are a subgroup of low-mass X-ray binaries consisting of a neutron star or a black hole and a companion low-mass star. SXTs exhibit a sudden outburst by increasing the luminosity from ∼ 1033 to ∼ 1036−38ergs1. After spending a few months in outburst, SXTs switch back to quiescence. Optical study of the binary system during the quiescence state of SXTs provides an opportunity to discriminate between BH binaries and neutron star binaries. The first part ot this research is composed of result of 10 years joint project between Hubble space telescope and Chandra, to study SXTs in M31. The other part of this thesis focused on the light curve of bright SXTs in M31. Disc irradiation is thought to be capable of explaining the global behaviour of the light curves of 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 (Lpeak > 1038ergs1) 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.format.mimetype application/pdf en
dc.language.iso en en
dc.publisher University College Cork en
dc.rights © 2014, Nakisa Nooraee en
dc.rights.uri http://creativecommons.org/licenses/by-nc-nd/3.0/ en
dc.subject Physics en
dc.title X-ray and optical studies of soft x-ray transients in M31 en
dc.type Doctoral thesis en
dc.type.qualificationlevel Doctoral en
dc.type.qualificationname PhD (Science) en
dc.internal.availability Full text available en
dc.check.info No embargo required en
dc.description.version Accepted Version
dc.contributor.funder Dublin Institute for Advanced Studies en
dc.description.status Not peer reviewed en
dc.internal.school Physics en
dc.check.type No Embargo Required
dc.check.reason No embargo required en
dc.check.opt-out Not applicable en
dc.thesis.opt-out false
dc.check.embargoformat Not applicable en
ucc.workflow.supervisor paulc@miranda.ucc.ie


Files in this item

This item appears in the following Collection(s)

Show simple item record

© 2014, Nakisa Nooraee Except where otherwise noted, this item's license is described as © 2014, Nakisa Nooraee
This website uses cookies. By using this website, you consent to the use of cookies in accordance with the UCC Privacy and Cookies Statement. For more information about cookies and how you can disable them, visit our Privacy and Cookies statement