Optical counterparts of cosmological gamma-ray bursts - Interaction with matter surrounding the parent galaxy

Details Optical counterparts of cosmological gamma-ray bursts - Interaction with matter surrounding the parent galaxy Optical counterparts of cosmological gamma-ray bursts - Interaction with matter surrounding the parent galaxy

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997azh....74..483b&link_type=abstract

Astronomicheskij Zhurnal, vol. 74, p. 483

Mathematics

Logic

5

Gamma Ray Bursts, Galaxies, Light Emission, Interstellar Matter, Light Curve, Visible Spectrum, Brightness Distribution, Astronomical Models, Ultraviolet Radiation, Density Distribution

Scientific paper

The interaction of emission from a cosmological gamma-ray burst with the interstellar medium surrounding the parent galaxy is investigated. It is shown that, irrespective of the particular model used to account for the formation of cosmological gamma-ray bursts, the brightest bursts should have counterparts at visual and ultraviolet wavelengths. The light curves of such counterparts are calculated for bursts with energies of 10 exp 51 and 10 exp 52 erg in interstellar media with different densities.

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