期刊
ASTROPHYSICAL JOURNAL
卷 633, 期 2, 页码 1027-1030出版社
IOP PUBLISHING LTD
DOI: 10.1086/466523
关键词
gamma rays : bursts; relativity; shock waves
The prompt localization of GRB 050525A by Swift allowed rapid follow-up of the afterglow. The observations revealed that the optical afterglow had a major rebrightening starting at similar to 0.01 days and ending at similar to 0.03 days, which was followed by an initial power-law decay. Here we show that this early emission feature can be interpreted as reverse-shock emission superposed by forward-shock emission in an interstellar medium environment. By fitting the observed data, we further constrain some parameters of the standard fireball-shock model: the initial Lorentz factor of the ejecta gamma(0) > 120, the magnetic energy fraction epsilon(B) > 4 x 10(-6), and the medium density n < 2 cm(-3). These limits are consistent with those from other very early optical afterglows observed so far. In principle, a wind environment for GRB 050525A is disfavored.
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