GRB 210121A: A Typical Fireball Burst Detected by Two Small Missions

被引:23
|
作者
Wang, Xiangyu Ivy [1 ]
Zheng, Xutao [2 ]
Xiao, Shuo [3 ,4 ]
Yang, Jun [1 ]
Liu, Zi-Ke [1 ]
Yang, Yu-Han [1 ]
Zou, Jin-Hang [5 ]
Zhang, Bin-Bin [1 ,6 ,7 ]
Zeng, Ming [2 ,8 ]
Xiong, Shao-Lin [3 ]
Feng, Hua [9 ]
Song, Xin-Ying [3 ]
Wen, Jiaxing [2 ]
Xu, Dacheng [2 ]
Chen, Guo-Yin [1 ,6 ]
Ni, Yang [1 ,6 ]
Zhang, Zi-Jian [1 ,6 ]
Wu, Yu-Xuan [1 ,6 ]
Cai, Ce [3 ,4 ]
Cang, Jirong [9 ]
Deng, Yun-Wei [1 ,6 ]
Gao, Huaizhong [2 ]
Kong, De-Feng [10 ]
Huang, Yue [3 ]
Li, Cheng-Kui [3 ]
Li, Hong [9 ]
Li, Xiao-Bo [3 ]
Liang, En-Wei [10 ]
Lin, Lin [11 ]
Liu, Yihui [2 ]
Long, Xiangyun [2 ]
Lu, Dian [2 ,8 ]
Luo, Qi [3 ,4 ]
Ma, Yong-Chang [1 ,6 ]
Meng, Yan-Zhi [1 ,6 ]
Peng, Wen-Xi [3 ]
Qiao, Rui [3 ]
Song, Li-Ming [3 ]
Tian, Yang [2 ,8 ]
Wang, Pei-Yuan [12 ]
Wang, Ping [3 ]
Wang, Xiang-Gao [10 ]
Xu, Sheng [1 ,6 ]
Yang, Dongxin [2 ]
Yin, Yi-Han [13 ]
Zeng, Weihe [2 ]
Zeng, Zhi [2 ,8 ]
Zhang, Ting-Jun [6 ,12 ]
Zhang, Yuchong [14 ]
Zhang, Zhao [1 ,6 ]
机构
[1] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Peoples R China
[2] Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China
[3] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, 19B Yuquan Rd, Beijing 100049, Peoples R China
[4] Chinese Acad Sci, Univ Chinese Acad Sci, Beijing 100049, Peoples R China
[5] Hebei Normal Univ, Coll Phys, Shijiazhuang 050024, Hebei, Peoples R China
[6] Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing, Peoples R China
[7] Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA
[8] Tsinghua Univ, Key Lab Particle & Radiat Imaging, Minist Educ, Beijing 100084, Peoples R China
[9] Tsinghua Univ, Dept Astron, Beijing 100084, Peoples R China
[10] Guangxi Univ, Sch Phys Sci & Technol, Guangxi Key Lab Relativist Astrophys, Nanning 530004, Peoples R China
[11] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
[12] Nanjing Univ, Kuang Yaming Honor Sch, Nanjing 210093, Peoples R China
[13] Nanjing Univ, Sch Phys, Nanjing 210093, Peoples R China
[14] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
来源
ASTROPHYSICAL JOURNAL | 2021年 / 922卷 / 02期
基金
中国国家自然科学基金;
关键词
GAMMA-RAY BURST; SPECTRAL LAGS; DOMINATED OUTFLOW; PEAK LUMINOSITY; GIANT FLARE; MAGNETAR; EVOLUTION; EMISSION; PHOTOSPHERES; 200415A;
D O I
10.3847/1538-4357/ac29bd
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Chinese CubeSat Mission, Gamma Ray Integrated Detectors (GRID), recently detected its first gamma-ray burst, GRB 210121A, which was jointly observed by the Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM). This burst is confirmed by several other missions, including Fermi and Insight-HXMT. We combined multimission observational data and performed a comprehensive analysis of the burst's temporal and spectral properties. Our results show that the burst is relatively special in its high peak energy, thermal-like low-energy indices, and large fluence. By putting it to the E (p) -E ( gamma,iso) relation diagram with assumed distance, we found that this burst can be constrained at the redshift range of [0.3, 3.0]. The thermal spectral component is also confirmed by the direct fit of the physical models to the observed spectra. Interestingly, the physical photosphere model also constrained a redshift of z similar to 0.3 for this burst, which helps us to identify a host galaxy candidate at such a distance within the location error box. Assuming that the host galaxy is real, we found that the burst can be best explained by the photosphere emission of a typical fireball with an initial radius of r (0) similar to 3.2 x 10(7) cm.
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页数:10
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