Discovery of a transient absorption edge in the X-ray spectrum of GRB 990705

被引:176
作者
Amati, L
Frontera, F
Vietri, M
in't Zand, JJM
Soffitta, P
Costa, E
Del Sordo, S
Pian, E
Piro, L
Antonelli, LA
Dal Fiume, D
Feroci, M
Gandolfi, G
Guidorzi, C
Heise, J
Kuulkers, E
Masetti, N
Montanari, E
Nicastro, L
Orlandini, M
Palazzi, E
机构
[1] CNR, Ist Tecnol & Studio Radiaz Extraterr, I-40129 Bologna, Italy
[2] Univ Ferrara, Dipartmento Fis, I-44100 Ferrara, Italy
[3] Terza Univ Roma, Dipartimento Fis, I-00146 Rome, Italy
[4] Space Res Org Netherlands, NL-3584 CA Utrecht, Netherlands
[5] Ist Fis Cosm Applicaz Informat, I-00133 Rome, Italy
[6] Osserv Astron Roma, I-00040 Rome, Italy
关键词
D O I
10.1126/science.290.5493.953
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
We report the discovery of a transient equivalent hydrogen column density with an absorption edge at similar to3.8 kiloelectron volts in the spectrum of the prompt x-ray emission of gamma-ray burst (GRB) 990705. This feature can be satisfactorily modeled with a photoelectric absorption by a medium Located at a redshift of similar to0.86 and with an iron abundance of similar to 75 times the solar one. The transient behavior is attributed to the strong ionization produced in the circumburst medium by the GRB photons. The high iron abundance points to the existence of a burst environment enriched by a supernova along the Line of sight. The supernova explosion is estimated to have occurred about 10 years before the burst. Our results agree with models in which GRBs originate from the collapse of very massive stars and are preceded by a supernova event.
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收藏
页码:953 / 955
页数:3
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