Swift observations of GRB 050128:: The early X-ray afterglow

被引:30
|
作者
Campana, S
Antonelli, LA
Chincarini, G
Covino, S
Cusumano, G
Malesani, D
Mangano, V
Moretti, A
Pagani, C
Romano, P
Tagliaferri, G
Capalbi, M
Perri, M
Giommi, P
Angelini, L
Boyd, P
Burrows, DN
Hill, JE
Gronwall, C
Kennea, JA
Kobayashi, S
Kumar, P
Mészáros, P
Nousek, JA
Roming, PWA
Zhang, B
Abbey, AF
Beardmore, AP
Breeveld, A
Goad, MR
Godet, O
Mason, KO
Osborne, JP
Page, KL
Poole, T
Gehrels, N
机构
[1] Osserv Astron Brera, INAF, I-23807 Merate, LC, Italy
[2] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Italy
[3] Univ Milan, Dipartimento Fis, I-20126 Milan, Italy
[4] INAF, Ist Astrofis Spaziale & Fis Cosm, Sez Palermo, I-90146 Palermo, Italy
[5] SISSA, ISAS, I-34014 Trieste, Italy
[6] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[7] ASI Sci Data Ctr, I-00044 Frascati, Rome, Italy
[8] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[9] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[10] Penn State Univ, Ctr Gravitat Wave Phys, University Pk, PA 16802 USA
[11] Univ Texas, Dept Astron, Austin, TX 78712 USA
[12] Univ Nevada, Dept Phys, Las Vegas, NV 89154 USA
[13] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
[14] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
来源
ASTROPHYSICAL JOURNAL | 2005年 / 625卷 / 01期
基金
美国国家航空航天局;
关键词
gamma rays : bursts; X-rays : individual (GRB 050128);
D O I
10.1086/430883
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Swift discovered GRB 050128 with the Burst Alert Telescope and promptly pointed its narrow field instruments to monitor the afterglow. X-ray observations started 108 s after the trigger time. The early decay of the afterglow is relatively flat, with a temporal decay modeled with a power-law index of similar to-0.3. A steepening occurs at later times (similar to 1500 s) with a power-law index of similar to-1.3. During this transition, the observed X- ray spectrum does not change. We interpret this behavior as either an early jet break or evidence of a transition from the fast cooling regime to the slow cooling regime in a wind environment.
引用
收藏
页码:L23 / L26
页数:4
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