Publication Date:
2019-04-02
Description:
The new method of statistical studying of cosmic gamma-ray bursts is presented based on the averaging of time profiles. The comparison is done between bright and dim events: while no differences were found between average flux curves, the hardness ratios pointed out the effect of hardness/brightness correlation.
Keywords:
ASTROPHYSICS
Type:
Advances in Space Research (ISSN 0273-1177); 15; 5; p. (5)131-(5)134
Format:
text
Permalink