Influence of the pulsar parameters on γ-ray burst afterglows

Details Influence of the pulsar parameters on γ-ray burst afterglows Influence of the pulsar parameters on γ-ray burst afterglows

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cha%26a..27..390x&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 27, Issue 4, p. 390-398.

Astronomy and Astrophysics

Astrophysics

Γ-Ray, Burst-Γ-Ray, Observation-Γ-Ray, Theory

Scientific paper

By applying the fireball model of γ-ray burst with a central pulsar, the radiation fluxes of the afterglows of two γ-ray bursts, GRB970228 and GRB000301c, are calculated. The results of the calculation agree very well with the observations. The differing characters of the light curves with a ``break'' in the optical waveband R of the afterglows of two bursts are interpreted, in terms of differing pulsar parameter values.

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