Hard X-rays and gamma rays from the Be star LSI +61-303

dc.contributor.author	Apparao, K. M. V
dc.date.accessioned	2008-02-29T11:11:42Z
dc.date.available	2008-02-29T11:11:42Z
dc.date.issued	2000
dc.identifier.citation	BASI, Vol. 28, No. 2, pp. 271 - 273	en
dc.identifier.uri	http://hdl.handle.net/2248/2100
dc.description.abstract	The hard x-ray flux resulting from inverse Compton scattering of photons from the Be star by the high energy electrons responsible for the radio emission, is calculated and compared with observation.	en
dc.format.extent	164480 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/2000BASI...28..271A	en
dc.subject	X-rays	en
dc.subject	Gamma rays	en
dc.subject	Be star	en
dc.title	Hard X-rays and gamma rays from the Be star LSI +61-303	en
dc.type	Article	en