When do internal shocks end and external shocks begin? Early-time broadband modeling of GRB 051111

Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/33872

Title:	When do internal shocks end and external shocks begin? Early-time broadband modeling of GRB 051111
Authors:	Butler,N. R.;Li,W.;Perley,D.;Huang,K. Y.;Urata,Y.;Prochaska,J. X.;Bloom,J. S.;Filippenko,A. V.;Foley,R. J.;Kocevski,D.;Chen,H. -W.;Qiu,Y.;Kuo,P. H.;Huang,F. Y.;Ip,W. H.;Tamagawa,T.;Onda,K.;Tashiro,M.;Makishima,K.;Nish
Contributors:	天文研究所
Keywords:	GAMMA-RAY BURST;AUTOMATIC IMAGING TELESCOPE;RELATIVISTIC BLAST WAVES;EARLY OPTICAL AFTERGLOW;HOST GALAXY;LIGHT-CURVE;DEPENDENT PHOTOIONIZATION;REFRESHED SHOCKS;IA SUPERNOVAE;DUSTY MEDIUM
Date:	2006
Issue Date:	2010-07-07 11:51:46 (UTC+8)
Publisher:	中央大學
Abstract:	Even with the renaissance in gamma-ray burst (GRB) research fostered by the Swift satellite, few bursts have both contemporaneous observations at long wavelengths and exquisite observations at later times across the electromagnetic spectrum. We present he
Relation:	ASTROPHYSICAL JOURNAL
Appears in Collections:	[天文研究所] 期刊論文

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