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pro vyhledávání: '"Chen, Aming"'
Autor:
Zhu, Jin-Ping, Liu, Liang-Duan, Yu, Yun-Wei, Mandel, Ilya, Hirai, Ryosuke, Zhang, Bing, Chen, Aming
Wolf-Rayet stars in close binary systems can be tidally spun up by their companions, potentially leaving behind fast-spinning highly-magnetized neutron stars, known as ``magnetars", after core collapse. These newborn magnetars can transfer rotational
Externí odkaz:
http://arxiv.org/abs/2405.01224
Autor:
Feng, Fabo, Rui, Yicheng, Du, Zhimao, Lin, Qing, Zhang, Congcong, Zhou, Dan, Cui, Kaiming, Ogihara, Masahiro, Yang, Ming, Lin, Jie, Cai, Yongzhi, Yang, Taozhi, Pang, Xiaoying, Jian, Mingjie, Li, Wenxiong, Guo, Hengxiao, Shi, Xian, Shi, Jianchun, Li, Jianyang, Guo, Kangrou, Yao, Song, Chen, Aming, Jia, Peng, Tan, Xianyu, Jenkins, James S., Jiang, Hongxuan, Zhang, Mingyuan, Li, Kexin, Xiao, Guangyao, Zheng, Shuyue, Xuan, Yifan, Zheng, Jie, He, Min, Jones, Hugh R. A., Song, Cuiying
Publikováno v:
AcASn, 2024, 65:34
Giant planets like Jupiter and Saturn, play important roles in the formation and habitability of Earth-like planets. The detection of solar system analogs that have multiple cold giant planets is essential for our understanding of planet habitability
Externí odkaz:
http://arxiv.org/abs/2404.07149
During the in-spiral stage of a compact binary, a wind bubble could be blown into interstellar medium, if the electromagnetic radiation due to the binary orbital motion is strong enough. Therefore, short gamma-ray bursts (SGRBs) due to double neutron
Externí odkaz:
http://arxiv.org/abs/1905.09663
Publikováno v:
The Astrophysical Journal Letters, 877:L21 (7pp), 2019 June 1
The accretion-induced collapse (AIC) of a white dwarf in a binary with a nondegenerate companion can sometimes lead to the formation of a rapidly rotating and highly magnetized neutron star (NS). The spin-down of this NS can drive a powerful pulsar w
Externí odkaz:
http://arxiv.org/abs/1904.11840
The formation of neutron stars (NSs), both from collapses of massive stars and mergers of compact objects, can be usually indicated by bright transients emitted from explosively-ejected material. In particular, if the newborn NSs can rotate at a mill
Externí odkaz:
http://arxiv.org/abs/1904.04440
Publikováno v:
The Astrophysical Journal Letters, 870:L23 (7pp), 2019 January 10
Super-Chandrasekhar remnants of double white dwarf mergers could sometimes collapse into a rapidly rotating neutron star (NS), accompanying with a mass ejection of a few times $0.01M_{\odot}$. Bright optical transient emission can be produced by the
Externí odkaz:
http://arxiv.org/abs/1812.06631
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