Beam Meets Target: A Model for Episodic Gamma-Ray Sources

Details Beam Meets Target: A Model for Episodic Gamma-Ray Sources Beam Meets Target: A Model for Episodic Gamma-Ray Sources

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.231..199a&link_type=abstract

Astrophysics and Space Science, Volume 231, Issue 1-2, pp. 199-202

Astronomy and Astrophysics

Astrophysics

Scientific paper

For an explanation of the TeVγ-ray episodes with duration ≤ 1 h observed from the X-ray binaries, we have suggested a model assuming that the beam of relativistic particles accelerated by the compact object meets the massive gas cloud ejected from the normal companion star. Here we present the time evolution of the resultingγ-ray spectra. We also discuss the possible application of the ’beam-meets-target’ model to the GRB, in particular those detected by EGRET, assuming that the accelerator is an isolated pulsar, and the target is a comet or asteroid.

Affiliated with

Also associated with

No associations

Rating

Beam Meets Target: A Model for Episodic Gamma-Ray Sources 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 Beam Meets Target: A Model for Episodic Gamma-Ray Sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Beam Meets Target: A Model for Episodic Gamma-Ray Sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-823517