Abstract
Gamma-ray bursts (GRBs) are short and intense flashes of γ-rays coming from deep space. GRBs were discovered more than a half century ago and now are observed across the whole electromagnetic spectrum from radio to very-high-energy gamma rays. They carry information about the powerful energy release during the final stage of stellar evolution, as well as properties of matter on the way to the observer. At present, space-based observatories detect on average approximately one GRB per day. In this review, we summarize key space and ground facilities that contribute to the GRB studies.
Funder
Ministry of Education, Universities and Research
RSF
European Structural and Investment Fund and the Czech Ministry of Education, Youth and Sports
Subject
General Physics and Astronomy
Cited by
6 articles.
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