GRB 990123: The Optical Flash and the Fireball Model

We compare the ongoing observations of the remarkable burst GRB990123 with the predictions of the afterglow theory. We show that the observations agree with the recent prediction that a reverse shock propagating into the ejecta would produce a very strong prompt optical flash. This reverse shock has also produced the 8.46GHz radio signal, observed after one day. The forward shock, which propagates into the ISM is the origin of the classical afterglow. It has produced the prompt X-ray signal as well as the late optical and IR emission. It would most likely produce a radio emission within the next few weeks. The observations suggest that the initial Lorentz factor of the ejecta was ∼ 200. Within factors of order unity, this crude model explains all current observations of GRB990123. Subject headings: γ-rays: burst; hydrodynamics; shock waves; relativity

Hali tarjima qilinmagan