Prompt and afterglow emission from the X-ray-rich GRB 981226 observed with Bepposax

被引:39
作者
Frontera, F
Antonelli, LA
Amati, L
Montanari, E
Costa, E
Dal Fiume, D
Giommi, P
Feroci, M
Gennaro, G
Heise, J
Masetti, N
Muller, JM
Nicastro, L
Orlandini, M
Palazzi, E
Pian, E
Piro, L
Soffitta, P
Stornelli, M
in't Zand, JJM
Frail, DA
Kulkarni, SR
Vietri, M
机构
[1] Univ Ferrara, Dipartimento Fis, I-44100 Ferrara, Italy
[2] CNR, Ist Tecnol & Studio Radiazioni Extraterr, I-40129 Bologna, Italy
[3] Osserv Astron Roma, I-00040 Monte Porzio Catone, Italy
[4] CNR, Ist Astrofis Spaziale, I-00133 Rome, Italy
[5] BeppoSAX Sci Data Ctr, I-00131 Rome, Italy
[6] BeppoSAX Operat Control Ctr, I-00131 Rome, Italy
[7] Space Res Org Netherlands, NL-3584 CA Utrecht, Netherlands
[8] CNR, Ist Fis Cosmica & Appl Informat, I-90146 Palermo, Italy
[9] Natl Radio Astron Observ, Socorro, NM 87801 USA
[10] CALTECH, Palomar Observ, Pasadena, CA 91125 USA
[11] Univ Roma Tre, Dipartimento Fis, I-00146 Rome, Italy
关键词
gamma rays : bursts; gamma rays : observations; shock waves; X-rays : general;
D O I
10.1086/309369
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss observations of the prompt X- and gamma-ray emission and X-ray afterglow from GRB 981226. This event has the weakest gamma-ray peak flux detected with the BeppoSAX Gamma-Ray Burst Monitor. It shows an isolated X-ray precursor and the highest X-ray to gamma-ray fluence ratio measured thus far with the BeppoSAX Wide Field Cameras. The event was followed up with the BeppoSAX Narrow Field Instruments, and the X-ray afterglow was detected up to 10 keV. The afterglow flux is observed to rise from a level below the sensitivity of the MECS/LECS telescopes up to a peak flux of (5 +/- 1) x 10(-13) ergs cm(-2) s(-1) in the 2-10 keV energy band. This rise is followed by a decline according to a power law with an index of 1.31(-0.39)(+0.44). We discuss these results in the light of the current GRB models.
引用
收藏
页码:697 / 703
页数:7
相关论文
共 37 条
[1]   BeppoSAX GRBM on-ground calibrations data analysis [J].
Amati, L ;
Cinti, MN ;
Feroci, M ;
Costa, E ;
Frontera, F ;
DalFiume, D ;
Collina, P ;
Nicastro, L ;
Orlandini, M ;
Palazzi, E ;
Rapisarda, M ;
Zavattini, G .
EUX, X-RAY, AND GAMMA-RAY INSTRUMENTATION FOR ASTRONOMY VIII, 1997, 3114 :176-185
[2]   BATSE OBSERVATIONS OF GAMMA-RAY BURST SPECTRA .1. SPECTRAL DIVERSITY [J].
BAND, D ;
MATTESON, J ;
FORD, L ;
SCHAEFER, B ;
PALMER, D ;
TEEGARDEN, B ;
CLINE, T ;
BRIGGS, M ;
PACIESAS, W ;
PENDLETON, G ;
FISHMAN, G ;
KOUVELIOTOU, C ;
MEEGAN, C ;
WILSON, R ;
LESTRADE, P .
ASTROPHYSICAL JOURNAL, 1993, 413 (01) :281-292
[3]  
BLOOM JS, 1998, GCN, P182
[4]   The medium-energy concentrator spectrometer on board the BeppoSAX X-ray astronomy satellite [J].
Boella, G ;
Chiappetti, L ;
Conti, G ;
Cusumano, G ;
DelSordo, S ;
LaRosa, G ;
Maccarone, MC ;
Mineo, T ;
Molendi, S ;
Re, S ;
Sacco, B ;
Tripiciano, M .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1997, 122 (02) :327-340
[5]   BeppoSAX, the wide band mission for X-ray astronomy [J].
Boella, G ;
Butler, RC ;
Perola, GC ;
Piro, L ;
Scarsi, L ;
Bleeker, JAM .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1997, 122 (02) :299-307
[6]  
CASTROTIRADO AJ, 1998, GCN, P172
[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]   Discovery of an X-ray afterglow associated with the gamma-ray burst of 28 February 1997 [J].
Costa, E ;
Frontera, F ;
Heise, J ;
Feroci, M ;
Zand, JI ;
Fiore, F ;
Cinti, MN ;
DalFiume, D ;
Nicastro, L ;
Orlandini, M ;
Palazzi, E ;
Rapisarda, M ;
Zavattini, G ;
Jager, R ;
Parmar, A ;
Owens, A ;
Molendi, S ;
Cusumano, G ;
Maccarone, MC ;
Giarrusso, S ;
Coletta, A ;
Antonelli, LA ;
Giommi, P ;
Muller, JM ;
Piro, L ;
Butler, RC .
NATURE, 1997, 387 (6635) :783-785
[9]  
DICIOLO L, 1998, 7074 IAU
[10]  
FIORE F, 1999, P 1 XMM WORKSH SCI X