The Effect of Non-thermal Protons on the High Energy Spectra of Black Hole Binaries

dc.contributor.author	Bhattacharyya, S
dc.contributor.author	Bhatt, N
dc.contributor.author	Misra, R
dc.contributor.author	Kaul, C. L
dc.date.accessioned	2008-06-19T07:11:55Z
dc.date.available	2008-06-19T07:11:55Z
dc.date.issued	2003
dc.identifier.citation	BASI, Vol. 31, No. 3&4, pp. 375 - 376	en
dc.identifier.uri	http://hdl.handle.net/2248/2456
dc.description.abstract	We investigate here the effect on the emitted spectrum of a black hole binary due to the presence of accelerated protons in the inner region of the accretion disk. Our study shows that e-e+ pairs and high energy -rays created in inelastic p - p collisions contribute mainly in the 1 - 10 MeV range and produce a broad feature in the spectrum in this energy range which can be verified by INTEGRAL and GLAST observations.	en
dc.format.extent	69305 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/2003BASI...31..375B	en
dc.subject	Protons	en
dc.subject	Black hole binaries	en
dc.title	The Effect of Non-thermal Protons on the High Energy Spectra of Black Hole Binaries	en
dc.type	Article	en