The strongly polarized afterglow of GRB 020405

被引:52
作者
Bersier, D
McLeod, B
Garnavich, PM
Holman, MJ
Grav, T
Quinn, J
Kaluzny, J
Challis, PM
Bower, RG
Wilman, DJ
Heyl, JS
Holland, ST
Hradecky, V
Jha, S
Stanek, KZ
机构
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[2] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
[3] Copernicus Astron Ctr, PL-00716 Warsaw, Poland
[4] Univ Durham, Dept Phys, Durham DH1 3LE, England
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
gamma rays : bursts; polarization;
D O I
10.1086/368158
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report polarization measurements and photometry for the optical afterglow of the gamma-ray burst GRB 020405. We measured a highly significant 9.9% polarization (in V band) 1.3 days after the burst and argue that it is intrinsic to the GRB. The light-curve decay is well fitted by a t(-1.72) power law; we do not see any evidence for a break between 1.24 and 4.3 days after the burst. We discuss these measurements in the light of several models of GRB afterglows.
引用
收藏
页码:L63 / L66
页数:4
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