The effects of the pulsar parameter on Gamma-ray burst afterglows

Details The effects of the pulsar parameter on Gamma-ray burst afterglows The effects of the pulsar parameter on Gamma-ray burst afterglows

Aug 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003acasn..44..240x&link_type=abstract

Acta Astronomica Sinica, vol. 44, no. 3, p. 240-248

Astronomy and Astrophysics

Astronomy

Pulsars: General, Gamma Ray: Bursts, Fireball Model, Afterglows

Scientific paper

The radiation flux of two gamma-ray bursts (GRB970228 and GRB000301) afterglows has been studied using the fireball model with a millisecond pulsar at the center, which turns out to be well consistent with the observation data. Our study also explains the break of the optical R-band of the light curve of these afterglows, and shows the pulsar parameters have significant effects on the light curve of the afterglows.

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