Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/2252
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dc.contributor.authorBeri, A.-
dc.date.accessioned2020-11-26T06:11:42Z-
dc.date.available2020-11-26T06:11:42Z-
dc.date.issued2019-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 482(4),pp. 4397-4407.en_US
dc.identifier.otherhttps://doi.org/10.1093/mnras/sty2975-
dc.identifier.urihttps://academic.oup.com/mnras/article/482/4/4397/5159493-
dc.identifier.urihttp://hdl.handle.net/123456789/2252-
dc.descriptionOnly IISERM authors are available in the record.-
dc.description.abstractWe present results from an observation of the low-mass X-ray binary 4U 1636–536 obtained with the LAXPC instrument aboard AstroSat. The observations of 4U 1636–536 made during the performance verification phase of AstroSat showed seven thermonuclear X-ray bursts in a total exposure of ∼65 ks over a period of about two consecutive days. Moreover, the light curve of 4U 1636–536 revealed the presence of a rare triplet of X-ray bursts, having a wait time of about 5.5 min between the second and the third bursts. We also present results from time-resolved spectroscopy performed during these seven X-ray bursts. In addition, we have also detected a transient quasi-periodic oscillation at ∼5 Hz. However, we did not find any evidence of kilo-hertz quasi-periodic oscillations and/or X-ray burst oscillations, perhaps due to the hard spectral state of the source during this observation.en_US
dc.language.isoenen_US
dc.publisherOxford Academicen_US
dc.subjectAccretionen_US
dc.subjectAccretion discsen_US
dc.subjectStars: neutronen_US
dc.titleThermonuclear X-ray bursts in rapid succession in 4U 1636–536 with AstroSat-LAXPCen_US
dc.typeArticleen_US
Appears in Collections:Research Articles

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