Multiwavelength afterglows of Gamma-Ray Bursts

Details Multiwavelength afterglows of Gamma-Ray Bursts Multiwavelength afterglows of Gamma-Ray Bursts

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003chjas...3..461p&link_type=abstract

Chinese Journal of Astronomy & Astrophysics, Vol. 3, Supplement, p. 461-471

Astronomy and Astrophysics

Astrophysics

1

Gamma-Ray Bursts, Supernovae

Scientific paper

Our knowledge of Gamma-Ray Burst (GRB) progenitors is based on three cases at relatively low redshift (between 0.01 and 0.2) in which the association with a supernova (SN) has been firmly established. In a number of higher redshift GRBs the presence of a SN has been suggested, although the properties of the SN could not be precisely determined. However, the study of several tens of multiwavelength afterglows has now provided evidence that GRBs are associated with star formation. The observational results which point to this connection are reviewed, and the high energy properties of afterglows and SNe are compared.

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