Testing the fireball/blastwave model by monitoring afterglows from soft gamma repeaters

Details Testing the fireball/blastwave model by monitoring afterglows from soft gamma repeaters Testing the fireball/blastwave model by monitoring afterglows from soft gamma repeaters

2005-02-22

arxiv.org/abs/astro-ph/0502452v1

J.Nanjing U.34:96,1998

Astronomy and Astrophysics

Astrophysics

A detailed version of astro-ph/9810449, published in 1998 in "Journal of Nanjing University" already; 6 figures, 11 pages

Scientific paper

The popular fireball/blastwave model of classical gamma-ray bursts is applied
to soft gamma-ray bursts. It is found that X-ray afterglows from strong events
may be above their quiescent levels for 40 -- 400 seconds. Optical afterglows
may also be detectable. By monitoring the three repeaters, we will have an
ideal way to check the fireball/blastwave model.

Affiliated with

Also associated with

No associations

Rating

Testing the fireball/blastwave model by monitoring afterglows from soft gamma repeaters 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 Testing the fireball/blastwave model by monitoring afterglows from soft gamma repeaters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Testing the fireball/blastwave model by monitoring afterglows from soft gamma repeaters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-471305