Detailed Study of the Variable Afterglow of GRB 060526

被引：0

作者：

Johannesson, G. ^{[1
,2
]}

Thone, C. C. ^{[3
]}

Kann, D. A. ^{[4
]}

Selj, J. H. ^{[5
]}

Jaunsen, A. ^{[5
]}

Fynbo, J. P. U. ^{[3
]}

Hanlon, L. ^{[6
]}

French, J. ^{[6
]}

机构：

[1] Univ Iceland, Inst Sci, Dunhaga 3, IS-107 Reykjavik, Iceland

[2] Stanford Univ, Hansen Expt Phys Lab, Stanford, CA 94305 USA

[3] Univ Copenhagen, Dark Cosmol Ctr, Niels Bohr Inst, DK-2100 Copenhagen, Denmark

[4] Thuringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany

[5] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway

[6] Univ Coll Dublin, Sch Phys, Dublin 4, Ireland

来源：

GAMMA-RAY BUSTS | 2009年 / 1133卷

关键词：

gamma rays: bursts; gamma rays: individual: GRB 060526; GAMMA-RAY BURST; 28; FEBRUARY; 1997; X-RAY; LIGHT CURVES; SWIFT ERA; ENERGY;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using one of the largest photometric datasets ever obtained for a GRB, we investigate the highly variable afterglow light curve of Gamma-Ray Burst 060526. The light curve shows clear deviations from a power-law behaviour which we attribute to energy injections. We fit the data to a numerical model including 6 energy injections which explains the full temporal behaviour of the light curve in many wavebands, ranging from NIR to X-rays.

引用

页码：221 / +

页数：2

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