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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4879
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dc.contributor.authorNaik, S.-
dc.contributor.authorAgrawal, P.C.-
dc.contributor.authorPaul, Biswajit-
dc.contributor.authorRao, A.R.-
dc.contributor.authorSeetha, S.-
dc.contributor.authorKasturirangan, K.-
dc.date.accessioned2012-07-12T11:47:52Z-
dc.date.available2012-07-12T11:47:52Z-
dc.date.issued2000-02-
dc.identifier.citationAstronomy and Astrophysics, 2000, Vol. 354, p928-942en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2289/4879-
dc.descriptionOpen Accessen
dc.description.abstractThe observations of a newly discovered X-ray transient source XTE J1748-288 were made in the energy band 2 - 18 keV with the Indian X-ray Astronomy Experiment(IXAE) on the IRS-P3 satellite during 1998, June 14-25. The source count rate declined gradually with an exponential decay time of 19 ± 1.6 days. The X-ray light curves showed no significant intensity variations on short time scales (<= 10s). The power density spectrum obtained from timing analysis of the data shows no quasi-periodic oscillations in the frequency range of 0.002 Hz to 5 Hz. From the observed X-ray and radio characteristics, it is suggested that the X-ray source in XTE J1748-288 is more likely to be a black hole rather than a neutron star.en
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000A%26A...354..938Nen
dc.rights2000 EDP Sciencesen
dc.titleObservation of X-ray transient XTE J1748−288 by the Indian X-ray astronomy experimenten
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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