Astron. Astrophys. Suppl. Ser.
Volume 138, Number 3, September 1999Gamma-Ray Bursts in the Afterglow Era Contents Rome, November 3-6, 1998
|Page(s)||451 - 452|
|Published online||15 September 1999|
Physical parameters of GRB 970508 from its afterglow synchrotron emission
Astronomical Institute "Anton Pannekoek"/CHEAF, Kruislaan 403, 1098 SJ, Amsterdam, The Netherlands
2 Dept. of Physics & Astronomy, SUNY, Stony Brook, NY, U.S.A.
3 Physics Department, UAH, Huntsville, AL 35899, U.S.A.
4 USRA at NASA/MSFC, Code ES-84, Huntsville AL 35812, U.S.A.
5 Institut de Radio Astronomie Millimétrique, 300 rue de la Piscine, F–38406 Saint-Martin d'Hères, France
6 NFRA, Radio Observatory, Postbus 2, 7990 AA, Dwingeloo, The Netherlands
7 Institute of Astronomy, Madingley Road, Cambridge, UK
Send offprint request to: T.J. Galama
Accepted: 4 May 1999
For the case of an adiabatically expanding blast wave, which is applicable to observed gamma-ray burst (GRB) afterglows at late times, we give expressions to infer the physical properties of the afterglow from the measured spectral features. We show that enough data exist for GRB 970508 to compute unambiguously the ambient density, cm-3, and the blast wave energy per unit solid angle, erg/4π sr. We also compute the energy density in electrons and magnetic field. We find that they are 12% and 9%, respectively, of the nucleon energy density.
Key words: gamma–rays: bursts / radiation mechanisms: non-thermal
© European Southern Observatory (ESO), 1999