Progress of the study of gamma-ray bursts (I): the observational feature and energy source.

Details Progress of the study of gamma-ray bursts (I): the observational feature and energy source. Progress of the study of gamma-ray bursts (I): the observational feature and energy source.

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pabei..13..206w&link_type=abstract

Prog. Astron., Vol. 13, No. 3, p. 206 - 219

Astronomy and Astrophysics

Astronomy

Gamma-Ray Bursts: Energy Spectra, Gamma-Ray Bursts: Space Distribution, Gamma-Ray Bursts: Energy Sources

Scientific paper

The authors discuss the observational features of gamma-ray bursts obtained in the past two decades, including temporal structures, energy spectra and spatial distribution. GRBs display very diverse temporal structures, their durations spanning from the shortest <1 s to the longest 1000 s, the average is about 15 s. The emission has been measured over a broad band of energies from 10 keV to 10 MeV, there are absorption and emission lines in some GRB spectra. The spatial distribution of GRBs appears isotropic. The authors also discuss some energy source mechanisms originated in the neutron star.

Affiliated with

Also associated with

No associations

Rating

Progress of the study of gamma-ray bursts (I): the observational feature and energy source. 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 Progress of the study of gamma-ray bursts (I): the observational feature and energy source., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Progress of the study of gamma-ray bursts (I): the observational feature and energy source. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-989991