Virgili 2013 超长暴GRR 091024a的观测
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Title: | GRB 091024A and the Nature of Ultra-long Gamma-Ray Bursts | |
Authors: | Virgili, F. J.; Mundell, C. G.; Pal'shin, V.; Guidorzi, C.; Margutti, R.; Melandri, A.; Harrison, R.; Kobayashi, S.; Chornock, R.; Henden, A.; Updike, A. C.; Cenko, S. B.; Tanvir, N. R.; Steele, I. A.; Cucchiara, A.; Gomboc, A.; Levan, A.; Cano, Z.; Mottram, C. J.; Clay, N. R.; Bersier, D.; Kopač, D.; Japelj, J.; Filippenko, A. V.; Li, W.; Svinkin, D.; Golenetskii, S.; Hartmann, D. H.; Milne, P. A.; Williams, G.; O'Brien, P. T.; Fox, D. B.; Berger, E. | |
Affiliation: | AA(Astrophysics Research Institute, Liverpool John Moores University, Liverpool, L3 5RF, UK | |
Publication: | The Astrophysical Journal, Volume 778, Issue 1, article id. 54, | |
Publication Date: | 11/2013 | |
Origin: | IOP | |
Astronomy Keywords: | gamma-ray burst: general, gamma-ray burst: individual: GRB 091024A | |
DOI: | 10.1088/0004-637X/778/1/54 | |
Bibliographic Code: | 2013ApJ...778...54V |
Abstract
We present a broadband study of gamma-ray burst (GRB) 091024A within the context of other ultra-long-duration GRBs. An unusually long burst detected by Konus-Wind (KW), Swift, and Fermi, GRB 091024A has prompt emission episodes covering ~1300 s, accompanied by bright and highly structured optical emission captured by various rapid-response facilities, including the 2 m autonomous robotic Faulkes North and Liverpool Telescopes, KAIT, S-LOTIS, and the Sonoita Research Observatory. We also observed the burst with 8 and 10 m class telescopes and determine the redshift to be z = 1.0924 ± 0.0004. We find no correlation between the optical and γ-ray peaks and interpret the optical light curve as being of external origin, caused by the reverse and forward shock of a highly magnetized jet (RB ≈ 100-200). Low-level emission is detected throughout the near-background quiescent period between the first two emission episodes of the KW data, suggesting continued central-engine activity; we discuss the implications of this ongoing emission and its impact on the afterglow evolution and predictions. We summarize the varied sample of historical GRBs with exceptionally long durations in gamma-rays (gsim1000 s) and discuss the likelihood of these events being from a separate population; we suggest ultra-long GRBs represent the tail of the duration distribution of the long GRB population.Bibtex entry for this abstract Preferred format for this abstract (see Preferences) |
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