- Conference date: 20–23 October 2008
- Location: Huntsville (Alabama)
The highly relativistic jets from collapsars are studied in the contect of the gamma‐ray burst (GRB). The angular energy distribution of the jets after the eruption from the stellar surface is well fitted by the smoothly broken power law. The distribution of the jets from light progenitor models is steeper than that of the jets injected in more massive progenitor stars. The cocoon property of the jet in the progenitor decides this characteristics of the jet.
MOST READ THIS MONTH
MOST CITED THIS MONTH
Article metrics loading...