The radiation mechanism of the soft gamma-ray repeater GB 790107

Details The radiation mechanism of the soft gamma-ray repeater GB 790107 The radiation mechanism of the soft gamma-ray repeater GB 790107

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994cha%26a..18...54z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 18, Issue 1, p. 54-59.

Astronomy and Astrophysics

Astrophysics

Neutron Star, Γ-Ray Bursts, Radiation Mechanism

Scientific paper

We assume that the soft gamma-ray repeater GB 790107 comes from a weakly magnetized (B ~ 108 G) neutron star, where shower-type accretion of cometary material results in an optically thick region on the surface of the star. The temperature distribution of the region is determined by the shock model. The blackbody radiation generated by the hot plasma of the region fits very well the observed spectrum of GB 790107. The distance of the burst source is found to be 1.35 ~ 13.5 pc.

Affiliated with

Also associated with

No associations

Rating

The radiation mechanism of the soft gamma-ray repeater GB 790107 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 The radiation mechanism of the soft gamma-ray repeater GB 790107, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The radiation mechanism of the soft gamma-ray repeater GB 790107 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-867023