2000/07/03 by E. Rol, R. A. M. J. Wijers, P. M. Vreeswijk +9 · 1 citation
Physics and Astronomy · #astro-ph
paper · pdf · doi:10.1086/317256
10 pages including 6 figures, accepted by ApJ. Uses aastex 5.0
arxiv created 2000/07/03 · arxiv updated 2009/12/01
We report the detection of significant polarization in the optical afterglow of GRB990712 on three instances 0.44, 0.70 and 1.45 days after the gamma-ray burst, with (P, theta) being (2.9% +- 0.4%, 121.1 degr +- 3.5 degr), (1.2% +- 0.4%, 116.2 degr +- 10.1 degr) and (2.2% +- 0.7%, 139.2 degr +- 10.4 degr) respectively. The polarization is intrinsic to the afterglow. The degree of polarization is not constant, and smallest at the second measurement. The polarization angle does not vary significantly during these observations. We find that none of the existing models predict such polarization variations at constant polarization angle, and suggest ways in which these models might be modified to accommodate the observed behavior of this afterglow.