dc.contributor.author |
Naik, S |
|
dc.contributor.author |
Agrawal, P. C |
|
dc.contributor.author |
Paul, B |
|
dc.contributor.author |
Rao, A. R |
|
dc.contributor.author |
Seetha, S |
|
dc.contributor.author |
Kasturirangan, K |
|
dc.date.accessioned |
2008-03-03T07:41:12Z |
|
dc.date.available |
2008-03-03T07:41:12Z |
|
dc.date.issued |
2000 |
|
dc.identifier.citation |
BASI, Vol. 28, No. 2, pp. 289 - 291 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2104 |
|
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.format.extent |
218812 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2000BASI...28..289N |
en |
dc.subject |
X-ray transient |
en |
dc.subject |
Black hole |
en |
dc.subject |
Accretion |
en |
dc.title |
The X-ray observation of newly discovered transient XTE J1748-288 by the Indian X-ray Astronomy Experiment |
en |
dc.type |
Article |
en |