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There is increasing evidence that massive stars may exhibit an enhanced mass loss shortly before their termination explosion. Some of them also indicate the enhancement of their circumstellar matter (CSM) is not spherically symmetric. Supernova (SN)
Externí odkaz:
http://arxiv.org/abs/2407.20720
The formation of black hole-neutron star (BH-NS) or BH-BH systems may be accompanied with special supernova (SN) signals, due to the accretion feedback from the companion BH. The additional heating, which is mainly attributed to the Blandford-Payne m
Externí odkaz:
http://arxiv.org/abs/2308.11913
The successful operation of dedicated detectors has brought us valuable information for understanding the central engine and the progenitor of gamma-ray bursts (GRBs). For instance, the giant X-ray and optical bumps found in some long-duration GRBs (
Externí odkaz:
http://arxiv.org/abs/2012.12036
Evidence for the central engine of gamma-ray bursts (GRBs) has been collected in the Neil Gehrels \emph{Swift} data. For instance, some GRBs show an internal X-ray plateau followed by very steep decay, which is difficult to be interpreted within the
Externí odkaz:
http://arxiv.org/abs/2005.00768
Autor:
Hu, Lei, Wu, Xuefeng, Andreoni, I., Ashley, Michael C. B., Cooke, J., Cui, Xiangqun, Du, Fujia, Dai, Zigao, Gu, Bozhong, Hu, Yi, Lu, Haiping, Li, Xiaoyan, Li, Zhengyang, Liang, Ensi, Liu, Liangduan, Ma, Bin, Shang, Zhaohui, Sun, Tianrui, Suntzeff, N. B., Tao, Charling, Uddin, Syed A., Wang, Lifan, Wang, Xiaofeng, Wen, Haikun, Xiao, Di, Xu, Jin, Yang, Ji, Yang, Shihai, Yuan, Xiangyan, Zhou, Hongyan, Zhang, Hui, Zhou, Jilin, Zhu, Zonghong
The LIGO detection of gravitational waves (GW) from merging black holes in 2015 marked the beginning of a new era in observational astronomy. The detection of an electromagnetic signal from a GW source is the critical next step to explore in detail t
Externí odkaz:
http://arxiv.org/abs/1710.05462
Akademický článek
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Publikováno v:
SCIENTIA SINICA Physica, Mechanica & Astronomica. 52:289512
Akademický článek
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Autor:
Wang, Jieshuang, Liu, Liangduan
Publikováno v:
Galaxies (2075-4434); Dec2021, Vol. 9 Issue 4, p104-104, 1p