Abstract
RINGO on the Liverpool Telescope has now measured the optical polarization of GRB 060418 (where a 2 sigma upper limit of P<8% was determined) and GRB 090102 (when a detection of P = 10 +/-1 % was made). We discuss the implications of these observations for the various competing models of GRB jet magnetization and describe a possible unified model that can explain both measurements.
Original language | English |
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Title of host publication | Proceedings of The Shocking Universe Conference held in San Servolo, 2009 |
Publication status | Published - Dec 2009 |