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
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
相关论文
共 24 条
[1]  
ANTONELLI LA, 2005, 2991 GCN
[2]  
BARTHELMY SD, 2005, IN PRESS SPACE SCI R
[3]   Gamma-ray burst energetics and the gamma-ray burst Hubble diagram: Promises and limitations [J].
Bloom, JS ;
Frail, DA ;
Kulkarni, SR .
ASTROPHYSICAL JOURNAL, 2003, 594 (02) :674-683
[4]   Swift X-Ray Telescope and very large telescope observations of the afterglow of GRB 041223 [J].
Burrows, DN ;
Hill, JE ;
Chincarini, G ;
Tagliaferri, G ;
Campana, S ;
Moretti, A ;
Romano, P ;
Malesani, D ;
Racusin, JL ;
Kobayashi, S ;
Zhang, B ;
Mészáros, P ;
O'Brien, PT ;
Willingale, R ;
Osborne, JP ;
Cusumano, G ;
Giommi, P ;
Angelini, L ;
Abbey, AF ;
Antonelli, LA ;
Beardmore, AP ;
Capalbi, M ;
Covino, S ;
D'Avanzo, P ;
Goad, MR ;
Kennea, JA ;
Morris, DC ;
Pagani, C ;
Page, KL ;
Stella, L ;
Nousek, JA ;
Wells, AA ;
Gehrels, N .
ASTROPHYSICAL JOURNAL, 2005, 622 (02) :L85-L88
[5]  
BURROWS DN, 2005, IN PRESS SPACE SCI R
[6]  
Bykov AM, 1996, ASTROPHYS J, V461, pL37, DOI 10.1086/309999
[7]   Wind interaction models for gamma-ray burst afterglows: The case for two types of progenitors [J].
Chevalier, RA ;
Li, ZY .
ASTROPHYSICAL JOURNAL, 2000, 536 (01) :195-212
[8]   Optical and NIR observations of the afterglow of GRB020813 [J].
Covino, S ;
Malesani, D ;
Tavecchio, F ;
Antonelli, LA ;
Arkharov, A ;
Di Paola, A ;
Fugazza, D ;
Ghisellini, G ;
Larionov, V ;
Lazzati, D ;
Mannucci, F ;
Masetti, N ;
Barrena, R ;
Benetti, S ;
Castro-Tirado, AJ ;
Alighieri, SD ;
Fiore, F ;
Frontera, F ;
Fruchter, A ;
Ghinassi, F ;
Gladders, M ;
Hall, PB ;
Israel, GL ;
Klose, S ;
Magazzù, A ;
Palazzi, E ;
Pedani, M ;
Pian, E ;
Romano, P ;
Stefanon, M ;
Stella, L .
ASTRONOMY & ASTROPHYSICS, 2003, 404 (01) :L5-L9
[9]  
COVINO S, 2005, 2999 GCN
[10]  
CUMMINGS J, 2005, 2992 GCN