Fitting the Crab Supernova with a Gamma-Ray Burst

被引:0
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作者
Ruffini, Remo [1 ,2 ,3 ,4 ]
Sigismondi, Costantino [1 ,3 ,5 ,6 ]
机构
[1] ICRANet, Int Ctr Relativist Astrophys Network, Coordinating Ctr, Piazzale Repubbl, I-65100 Pescara, Italy
[2] ICRANet, Int Ctr Relativist Astrophys Network, Coordinating Ctr, F-06000 Nice, France
[3] Sapienza Univ Roma, ICRA Int Ctr Relativist Astrophys, Dept Fis, Ple Aldo Moro 5, I-00185 Rome, Italy
[4] INAF Natl Inst Astrophys, Viale Parco Mellini 84, I-00136 Rome, Italy
[5] APRA-Ateneo Pontificio Regina Apostolorum, Via Aldobrandeschi 190, I-00163 Rome, Italy
[6] ITIS Galileo Ferraris, via Fonteiana 111, I-00152 Rome, Italy
关键词
supernova (SN1054); gamma-ray burst (GRB190114C); binary-driven hypernova;
D O I
10.3390/universe10070275
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Here, we reconsider the historical data, assuming a gamma-ray burst (GRB) as its source. A Supernova correlated with the GRB explains well the fading time observed by the ancient Chinese astronomers in the daytime and the nighttime, while the GRB power law explains the present X-rays and GeV emission of the Crab. On the grounds of a recent understanding of the first episode of binary-driven hypernova GRB (BDHN GRB) in terms of the collapse of a ten solar masses core, we propose the possible identification of the real Supernova event at an earlier time than Chinese chronicles. This work allows a new understanding of the significance of historical astronomical observations, including a fireball due to gamma-ray air shower observation and a plague of acute radiation syndrome, documented with several thousands of victims in the Eurasian area (Egypt, Iraq, and Syria).
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页数:10
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