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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2104
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dc.contributor.authorNaik, S-
dc.contributor.authorAgrawal, P. C-
dc.contributor.authorPaul, B-
dc.contributor.authorRao, A. R-
dc.contributor.authorSeetha, S-
dc.contributor.authorKasturirangan, K-
dc.date.accessioned2008-03-03T07:41:12Z-
dc.date.available2008-03-03T07:41:12Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 289 - 291en
dc.identifier.urihttp://hdl.handle.net/2248/2104-
dc.description.abstractThe observations of X-ray transient XTE J1748-288 were made in the energy band 2 - 18 keV with the Indian X-ray astronomy experiment (IXAE) during 1998, June 14-25 with total useful exposure of 27,100 second for 1 sec integration mode and 15,440 sec for the 0.1 sec mode. The X-ray light curves showed no significant intensity variations on short time scale (< 10s). The power density spectrum obtained from timing analysis of the data show no quasi-periodic oscillations in the frequency range of 0.001 Hz to 5 Hz. From the observed X-ray characteristics it is difficult to infer the nature of the X-ray source.en
dc.format.extent218812 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..289Nen
dc.subjectX-ray transienten
dc.subjectBlack holeen
dc.subjectAccretionen
dc.titleThe X-ray observation of newly discovered transient XTE J1748-288 by the Indian X-ray Astronomy Experimenten
dc.typeArticleen
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