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DC Field | Value | Language |
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dc.contributor.author | Naik, S. | - |
dc.contributor.author | Agrawal, P.C. | - |
dc.contributor.author | Paul, Biswajit | - |
dc.contributor.author | Rao, A.R. | - |
dc.contributor.author | Seetha, S. | - |
dc.contributor.author | Kasturirangan, K. | - |
dc.date.accessioned | 2012-07-14T06:27:35Z | - |
dc.date.available | 2012-07-14T06:27:35Z | - |
dc.date.issued | 2000-06 | - |
dc.identifier.citation | Bulletin of the Astronomical Society of India, Vol.28, p289-291 | en |
dc.identifier.issn | 0304-9523 | - |
dc.identifier.uri | http://hdl.handle.net/2289/4893 | - |
dc.description | Restricted Access | en |
dc.description.abstract | The 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.language.iso | en | en |
dc.publisher | The Astronomical Society of India | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/2000BASI...28..289N | en |
dc.rights | 2000 The Astronomical Society of India | en |
dc.subject | X-ray transient | en |
dc.subject | black holes | en |
dc.subject | accretion | en |
dc.title | X-ray observation of newly discovered transient XTE J1748-288 by the Indian X-ray astronomy experiment | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
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File | Description | Size | Format | |
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2000_BASI_V28__p289.pdf Restricted Access | Restricted Access | 217.79 kB | Adobe PDF | View/Open Request a copy |
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