Observations of the Optical Afterglow of GRB 050319: The Wind-to-ISM Transition in View
A. KambleRaman Research Institute, Bangalore 560-080, IndiaL. ResmiJoint Astronomy Programme, Indian Institute of Science, Bangalore 560-012, IndiaKuntal MisraAryabhatta Research Institute of Observational Sciences, Manora Peak, Nainital 263-129, India
2007en
ABI
Annotatsiya
One of the long standing questions in astrophysics is the progenitors of Gamma Ray Bursts (GRBs). Collapse of a massive star is one of the most favoured progenitors of the long GRBs. Evidence for a massive star being a GRB progenitor may be obtained in two different ways, both using observations of GRB afterglows. (1) Supernova (SN) component
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