Present status of hard X-ray astronomy

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DC Field	Value	Language
dc.contributor.author	Rao, A. R	-
dc.date.accessioned	2007-04-23T05:56:20Z	-
dc.date.available	2007-04-23T05:56:20Z	-
dc.date.issued	1993	-
dc.identifier.citation	BASI, Vol. 21, pp. 303-312	en
dc.identifier.uri	http://hdl.handle.net/2248/1492	-
dc.description.abstract	The recent observational results obtained in the energy range of 15-150 keV from balloon and satellite borne instruments are reviewed. The detection of cyclotron line features in several X-ray binaries, hard X-ray spectra and variability of black hole candidates and the hard X-ray imaging of Galactic center region are discussed. The need for developing low background, good resolution, high sensitivity hard X-ray detectors is stressed and the developments carried out in this regard at Tata Institute of Fundamental Research (TIFR) and elsewhere are briefly outlined	en
dc.format.extent	868548 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	X-ray Astronomy	en
dc.subject	Galactic center	en
dc.title	Present status of hard X-ray astronomy	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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