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

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

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003basi...31..375b&link_type=abstract

Bulletin of the Astronomical Society of India, vol. 31, p.375-376

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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