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Variable polarization in the optical afterglow of GRB021004

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journal contribution
posted on 2012-10-24, 09:22 authored by E. Rol, R. A. M. J. Wijers, J. P. U. Fynbo, J. Hjorth, J. Gorosabel, M. P. Egholm, J. M. C. Ceron, A. J. Castro-Tirado, L. Kaper, N. Masetti, E. Palazzi, E. Pian, N. Tanvir, P. Vreeswijk, C. Kouveliotou, P. Moller, H. Pedersen, A. S. Fruchter, J. Rhoads, I. Burud, I. Salamanca, Van den Heuvel E. P. J.
We present polarimetric observations of the afterglow of gamma-ray burst (GRB) 021004, obtained with the Nordic Optical Telescope (NOT) and the Very Large Telescope (VLT) between 8 and 17 hours after the burst. Comparison among the observations shows a 45 degree change in the position angle from 9 hours after the burst to 16 hours after the burst, and comparison with published data from later epochs even shows a 90 degree change between 9 and 89 hours after the burst. The degree of linear polarization shows a marginal change, but is also consistent with being constant in time. In the context of currently available models for changes in the polarization of GRBs, a homogeneous jet with an early break time of $t_{\rm b} \approx 1$ day provides a good explanation of our data. The break time is a factor 2 to 6 earlier than has been found from the analysis of the optical light curve. The change in the position angle of the polarization rules out a structured jet model for the GRB.

History

Citation

Astronomy & Astrophysics, 2003, 405 (3), pp. L23-L27

Version

  • VoR (Version of Record)

Published in

Astronomy & Astrophysics

Publisher

EDP Sciences for European Southern Observatory (ESO)

issn

0004-6361

Copyright date

2003

Available date

2012-10-24

Publisher version

http://www.aanda.org/articles/aa/abs/2003/27/aafc184/aafc184.html

Language

English