Abstract
We present the first high-resolution observations of the optical afterglow of a gamma-ray burst. The spectra show that the matter of the host galaxy in the circumburst region is complex, with many components contributing to each system. Also the presence of low- and high-ionisation lines allows rather strong constraints on the gas ionisation parameters of the various components to be derived. These can be interpreted as density fluctuations on top of a regular R-2 wind density profile.
| Original language | English |
|---|---|
| Pages (from-to) | 783-786 |
| Number of pages | 4 |
| Journal | Nuovo Cimento della Societa Italiana di Fisica C |
| Volume | 28 |
| Issue number | 4-5 |
| State | Published - 2005 |
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