Abstract
We present BVRI light curves of the afterglow of GRB000301C, one of the brightest ever detected at a day time scale interval after GRB trigger. The monitoring started 1.5 days after the GRB and ended one month later. Inspection of the extremely well sampled R band light curve and comparison with BVI data has revealed complex behavior, with a long term flux decrease and various short time scale features superimposed. These features are uncommon among other observed afterglows. and might trace either intrinsic variability within the relativistic shock (re-acceleration and re-energization) or inhomogeneities in the medium in which the shock propagates.
| Original language | English |
|---|---|
| Journal | Astronomy and Astrophysics |
| Volume | 359 |
| Issue number | 3 |
| Pages (from-to) | L23-L26 |
| ISSN | 0004-6361 |
| Publication status | Published - 2000 |
Keywords
- gamma rays : bursts
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