dc.contributor.author |
Rana, V. R |
|
dc.contributor.author |
Singh, K. P |
|
dc.date.accessioned |
2008-06-06T07:37:24Z |
|
dc.date.available |
2008-06-06T07:37:24Z |
|
dc.date.issued |
2003 |
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dc.identifier.citation |
BASI, Vol. 31, No. 3&4, pp. 347 - 349 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2414 |
|
dc.description.abstract |
Results from hard X-ray observations with RXTE of 5 Polar systems-V2301 Oph, V1432 Aql, EP Dra, GG Leo and V834 Cen, and an Intermediate Polar TV Col are presented. An improved ephemeris for V2301 Oph using mid-eclipse timings has been derived. V1432 Aql shows structured lightcurve containing several prominent peaks and dips. A likely eclipse of X-ray source in EP Dra is observed for the first time. The X-ray emission in EP Dra and GG Leo is found to be consistent with a single pole accretion. V 834 Cen was observed to be bright during 1996-1998, but was 16 times fainter during 2002 observations. The power spectrum of TV Col shows a significant power at frequencies corresponding to the spin period (1910s) and the binary period (5.5hr) and their side-bands, thereby suggesting that both the stream-fed and disk-fed accretion components are present in TV Col. |
en |
dc.format.extent |
92213 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2003BASI...31..347R |
en |
dc.subject |
Binaries: close |
en |
dc.subject |
Novae |
en |
dc.subject |
Cataclysmic variables |
en |
dc.subject |
Stars: individual |
en |
dc.subject |
TV col |
en |
dc.subject |
X-rays: stars |
en |
dc.title |
RXTE Observations of Magnetic Cataclysmic Variables |
en |
dc.type |
Article |
en |