High-Energy Emission from Accreting Black Holes with High-Mass Donor Stars

Details High-Energy Emission from Accreting Black Holes with High-Mass Donor Stars High-Energy Emission from Accreting Black Holes with High-Mass Donor Stars

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..33..122v&link_type=abstract

Massive Stars: Fundamental Parameters and Circumstellar Interactions (Eds. P. Benaglia, G. L. Bosch, & C. E. Cappa) Revista Mexi

Physics

Black Hole Physics, Gamma Rays: Theory, Stars: Early-Type

Scientific paper

We present an analysis of the interactions of a distribution of
relativistic protons under the typical conditions of the corona
surrounding an accreting black hole. The model is applied to a concrete
binary system with a high-mass donor star: the classical source Cygnus
X-1.

Affiliated with

Also associated with

No associations

Rating

High-Energy Emission from Accreting Black Holes with High-Mass Donor Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with High-Energy Emission from Accreting Black Holes with High-Mass Donor Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-Energy Emission from Accreting Black Holes with High-Mass Donor Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1807676