Abstract
Swift unprecedented fast follow-up observations of gamma-ray bursts have allowed us to discover a new feature of GRB afterglows: a phase of shallow decay, usually attributed to energy injection in the burst ejecta, which can last for several thousands of seconds both in the X-ray and optical bands. Here I discuss this phase in the case of Swift GRBs 050401, 050801 and 050802.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1471-1473 |
| Number of pages | 3 |
| Journal | Nuovo Cimento della Societa Italiana di Fisica B |
| Volume | 121 |
| Issue number | 12 |
| DOIs | |
| State | Published - Dec 2006 |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy