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of 1 141
pro vyhledávání: '"Liu Wei-Min"'
Publikováno v:
MNRAS 523, 907 (2023)
The disc instability mechanism (DIM) is widely accepted to account for the transient behaviour of dwarf novae (DNe), which experience short outbursts separated by long quiescence. The duty cycle (the ratio between the outburst duration and the recurr
Externí odkaz:
http://arxiv.org/abs/2308.08298
Publikováno v:
A&A 668, A80 (2022)
Ultracompact cataclysmic variables (CVs) of the AM CVn type are deemed to be important verification sources for the future space gravitational wave detectors such as the Laser Interferometer Space Antenna (LISA). We model the present-day Galactic pop
Externí odkaz:
http://arxiv.org/abs/2210.08434
Autor:
Zhang, Yi-Wang, Zhao, Chang, Su, Bo-Jing, Lin, Wei-Zheng, Liu, Wei-Min, Liang, Jing, Shao, Chun-Kui, Cheng, Na, Chen, Jian-Ning
Publikováno v:
In Annals of Diagnostic Pathology December 2024 73
Publikováno v:
In Ocean Engineering 1 December 2024 313 Part 3
Publikováno v:
In Ocean Engineering 15 June 2024 302
Autor:
Jiang, L., Wang, Na, Chen, Wen-Cong, Liu, Wei-Min, Leng, Chun-wei, Yuan, Jian-Ping, Qian, Xiang-Li
PSR J$1946+3417$ is a millisecond pulsar (MSP) with a spin period $P\simeq3.17\rm~ms$. Harbored in a binary with an orbital period $P_{\rm b}\simeq27$ days, the MSP is accompanied by a white dwarf (WD). The masses of the MSP and the WD were determine
Externí odkaz:
http://arxiv.org/abs/2106.05717
The space gravitational wave (GW) detector Laser Interferometer Space Antenna (LISA) that was planed to launch in the early 2030s is to detect the low-frequency GW signals in the Galaxy. AM CVn stars were generally thought to be important low-frequen
Externí odkaz:
http://arxiv.org/abs/2101.09850
Publikováno v:
In Ocean Engineering 15 February 2024 294
Akademický článek
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Publikováno v:
In Ocean Engineering 15 October 2023 286 Part 1