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Price PA Fox DW Kulkarni SR Peterson BA Schmidt BP Soderberg AM Yost SA Berger E Djorgovski SG Frail DA Harrison FA Sari R Blain AW Chapman SC 《Nature》2003,423(6942):844-847
Past studies of cosmological gamma-ray bursts (GRBs) have been hampered by their extreme distances, resulting in faint afterglows. A nearby GRB could potentially shed much light on the origin of these events, but GRBs with a redshift z 相似文献
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Fox DW Yost S Kulkarni SR Torii K Kato T Yamaoka H Sako M Harrison FA Sari R Price PA Berger E Soderberg AM Djorgovski SG Barth AJ Pravdo SH Frail DA Gal-Yam A Lipkin Y Mauch T Harrison C Buttery H 《Nature》2003,422(6929):284-286
Observations of the long-lived emission--or 'afterglow'--of long-duration gamma-ray bursts place them at cosmological distances, but the origin of these energetic explosions remains a mystery. Observations of optical emission contemporaneous with the burst of gamma-rays should provide insight into the details of the explosion, as well as into the structure of the surrounding environment. One bright optical flash was detected during a burst, but other efforts have produced negative results. Here we report the discovery of the optical counterpart of GRB021004 only 193 seconds after the event. The initial decline is unexpectedly slow and requires varying energy content in the gamma-ray burst blastwave over the course of the first hour. Further analysis of the X-ray and optical afterglow suggests additional energy variations over the first few days. 相似文献
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