Gamma-Ray Burst Afterglows with ALMA

被引：0

作者：

Urata, Yuji ^{[1
]}

Huang, Kuiyun ^{[2
]}

Takahashi, Satoko ^{[3
,4
]}

机构：

[1] Natl Cent Univ, Inst Astron, Zhongli, Taiwan

[2] Natl Taiwan Normal Univ, Dept Math & Sci, Zhongli, Taiwan

[3] Joint ALMA Observ, Santiago, Chile

[4] Natl Astron Observ Japan, Mitaka, Tokyo, Japan

来源：

REVOLUTION IN ASTRONOMY WITH ALMA: THE THIRD YEAR | 2015年 / 499卷

关键词：

SHOCK;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present multi-wavelength observations including sub-millimeter follow-ups for two GRB afterglows. The rapid SMA and multi-wavelength observations for GRB120326A revealed their complex emissions as the synchrotron self-inverse Compton radiation from reverse shock. The observations including ALMA for GRB131030A also showed the significant X-ray excess from the standard forward shock synchrotron model. Based on these results, we also discuss further observations for (A) constraining of the mass of progenitor with polarization, (B) the first confirmation of GRB jet collimation, and (C) revealing the origin of optically dark GRBs.

引用

页码：339 / 340

页数：2

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