Multicolor shallow decay and chromatic breaks in the GRB 050319 optical afterglow

Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/33838

Title:	Multicolor shallow decay and chromatic breaks in the GRB 050319 optical afterglow
Authors:	Huang,K. Y.;Urata,Y.;Kuo,P. H.;Ip,W. H.;Ioka,K.;Aoki,T.;Chen,C. W.;Chen,W. P.;Isogai,M.;Lin,H. C.;Makishima,K.;Mito,H.;Miyata,T.;Nakada,Y.;Nishiura,S.;Onda,K.;Qiu,Y.;Soyano,T.;Tamagawa,T.;Tarusawa,K.;Tashiro,M.;Yo
Contributors:	天文研究所
Keywords:	GAMMA-RAY BURSTS;THEORETICAL IMPLICATIONS;ENERGY INJECTION;LIGHT CURVES;JETS;EFFICIENCY;EMISSION;COLORS
Date:	2007
Issue Date:	2010-07-07 11:50:32 (UTC+8)
Publisher:	中央大學
Abstract:	Multiwavelength observations of the optical afterglow of GRB 050319 were performed from 1.31 to 9.92 hr after the burst. Our R-band light curves, combined with other published data, can be described by the smooth broken power-law function, with alpha(1) =
Relation:	ASTROPHYSICAL JOURNAL
Appears in Collections:	[Graduate Institute of Astronomy] journal & Dissertation

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