Understanding the behavior of energy X-rays from the black hole candidate GRS 1915+105

dc.contributor.author	Nandi, A
dc.contributor.author	Chakrabarti, S. K
dc.date.accessioned	2008-06-18T11:18:17Z
dc.date.available	2008-06-18T11:18:17Z
dc.date.issued	2002
dc.identifier.citation	BASI, Vol. 30, No. 1, pp. 327 - 330	en
dc.identifier.uri	http://hdl.handle.net/2248/2444
dc.description.abstract	Black Hole candidate GRS 1915+105 shows a very interesting behaviour at high energy X-rays. For instance, it shows quasi-Periodic Oscillations (QPO) only at high energies. Also the spectral slopes at high energies vary and carry information about the winds and jets produced at the centrifugal barrier. We discuss these aspects of the observations with explanation from the present theoretical models.	en
dc.format.extent	352005 bytes
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/2002BASI...30..327N	en
dc.subject	X-rays	en
dc.subject	Stars	en
dc.subject	Accretion	en
dc.subject	Outflows	en
dc.subject	Black Hole Physics	en
dc.subject	GRS 1915+105	en
dc.title	Understanding the behavior of energy X-rays from the black hole candidate GRS 1915+105	en
dc.type	Article	en