Constraints on the optical counterpart of GBS0526-66

Details Constraints on the optical counterpart of GBS0526-66 Constraints on the optical counterpart of GBS0526-66

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stin...8925084b&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Galactic Radiation, Gamma Ray Astronomy, Gamma Ray Bursts, Mathematical Models, Modulation, Supernova Remnants

Scientific paper

The upper limits to the magnitude of the pulsed optical emission of the object causing the L979b gamma ray burst are derived from the survey of the N49 supernova remnant carried out with a 50 cm telescope. The possibility that part of the emission is modulated, leading to a lower limit to the magnitude of a periodic component of 19.4 mV is discussed. The results are discussed in the framework of theoretical models of gamma ray bursts.

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