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IS THE LINE-LIKE OPTICAL AFTERGLOW SED OF GRB 050709 DUE TO A FLARE?
Liu, Cong; Jin, Zhi-Ping; Wei, Da-Ming
2016
发表期刊ASTROPHYSICAL JOURNAL
卷号833期号:2页码:234
摘要Recently, Jin et al. reanalyzed the optical observation data of GRB 050709 and reported a line-like spectral energy distribution (SED) component observed by the Very Large Telescope at t similar to 2.5 days after the trigger of the burst, which had been interpreted as a broadened line signal arising from a macronova dominated by an. iron group. In this work, we show that an optical flare origin of such a peculiar optical SED is still possible. Interestingly, even in such a model, an "unusual" origin of the late-time long-lasting Hubble Space Telescope F814W-band emission is still needed and a macronova/kilonova is the natural interpretation.
文献类型期刊论文
条目标识符http://libir.pmo.ac.cn/handle/332002/17073
专题期刊(老文献)
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Liu, Cong,Jin, Zhi-Ping,Wei, Da-Ming. IS THE LINE-LIKE OPTICAL AFTERGLOW SED OF GRB 050709 DUE TO A FLARE?[J]. ASTROPHYSICAL JOURNAL,2016,833(2):234.
APA Liu, Cong,Jin, Zhi-Ping,&Wei, Da-Ming.(2016).IS THE LINE-LIKE OPTICAL AFTERGLOW SED OF GRB 050709 DUE TO A FLARE?.ASTROPHYSICAL JOURNAL,833(2),234.
MLA Liu, Cong,et al."IS THE LINE-LIKE OPTICAL AFTERGLOW SED OF GRB 050709 DUE TO A FLARE?".ASTROPHYSICAL JOURNAL 833.2(2016):234.
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