Zobrazeno 61 - 70
of 1 738
pro vyhledávání: '"Liu, Dongdong"'
Publikováno v:
In Industrial Crops & Products 15 December 2023 206
Autor:
Liu, Dongdong, Zhang, Zhenyu, Zhou, Hongxiu, Deng, Xingqiao, Shi, Chunjing, Meng, Fanning, Yu, Zhibin, Feng, Junyuan
Publikováno v:
In Applied Surface Science 15 December 2023 640
Autor:
Tang, Jinping, Sun, Guangyi, Feng, Xinbin, Liu, Dongdong, Fei, Yingxiang, Shang, Jing, Finfrock, Y. Zou, Liu, Peng
Publikováno v:
In Chemical Engineering Journal 1 December 2023 477
Publikováno v:
In Diamond & Related Materials December 2023 140 Part B
Autor:
He, Yunfei, Li, Xinyu, Liu, Dongdong, Fu, Wenbo, Su, Qiang, Zhong, Bo, Xia, Long, Huang, Xiaoxiao
Publikováno v:
In Applied Surface Science 1 December 2023 639
Autor:
Ma, Yan, Wu, Haitao, Guo, Qinglong, Dai, Xingliang, Wang, Peisan, Zhang, Wei, Liu, Dongdong, Chen, Xulin, Qian, Haisheng, Wang, Xianwen
Publikováno v:
In Journal of Colloid And Interface Science December 2023 651:47-58
Publikováno v:
In Mechanical Systems and Signal Processing 1 January 2025 222
Accretion induced collapse (AIC) may be responsible for the formation of some interesting neutron star binaries, e.g., millisecond pulsars, intermediate-mass binary pulsars, etc. It has been suggested that oxygen-neon white dwarfs (ONe WDs) can incre
Externí odkaz:
http://arxiv.org/abs/2008.00866
Autor:
Wang, Bo, Liu, Dongdong
Publikováno v:
Res. Astron. Astrophys., Volume 20, Issue 9, id.135 (2020)
The accretion-induced collapse (AIC) scenario was proposed 40 years ago as an evolutionary end state of oxygen-neon white-dwarfs (ONe WDs), linking them to the formation of neutron star (NS) systems. However, there has been no direct detection of any
Externí odkaz:
http://arxiv.org/abs/2005.01880
The formation of single neutron-stars from double white-dwarf mergers via accretion-induced collapse
Autor:
Liu, Dongdong, Wang, Bo
Publikováno v:
MNRAS, 494, 3422 (2020)
The merging of double white dwarfs (WDs) may produce the events of accretion-induced collapse (AIC) and form single neutron stars (NSs). Meanwhile, it is also notable that the recently proposed WD+He subgiant scenario has a significant contribution t
Externí odkaz:
http://arxiv.org/abs/2004.03157