Abstract
We present a relation that links the flux, the distance arid the decay index of the GRB afterglows. We actualized it in X-ray using BeppoSAX, XMM-Newton, Chandra and SWIFT observations. We discuss the similar behaviour found recently at optical wavelengths using SWIFT afterglow data. We present evidences that this relation can be used to estimate the source distance as well as the optical extinction.
Original language | English |
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Pages (from-to) | 1377-1381 |
Number of pages | 5 |
Journal | Il Nuovo Cimento B |
Volume | 121 |
Issue number | 10-11 |
DOIs | |
Publication status | Published - 2006 |
Externally published | Yes |
Event | Workshop on Swift and GRBs - Unveiling the Relativistic University - Venice, Italy Duration: 5 Jun 2006 → 9 Jun 2006 |