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	Determination of wind-fed model parameters of neutron stars in high-mass X-ray binaries 期刊论文 OAI收割 PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, 2022, 卷号: 39, 页码: e040 作者: Taani, Ali; Karino, Shigeyuki; Song, Liming; Zhang, Chengmin; Chaty, Sylvain \| 收藏 \| 浏览/下载：10/0 \| 提交时间：2023/11/10
	On the wind accretion model of GX 301-2 期刊论文 OAI收割 Journal of Physics: Conference Series, 2019, 卷号: 1258, 期号: 1 作者: Taani,Ali; Karino,Shigeyuki; Song,Liming; Mardini,Mohammad; Al-Wardat,Mashhoor \| 收藏 \| 浏览/下载：17/0 \| 提交时间：2020/03/10
	On the possibility of disk-fed formation in supergiant high-mass X-ray binaries 期刊论文 OAI收割 RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2019, 卷号: 19, 期号: 1, 页码: 8 作者: Taani, Ali; Karino, Shigeyuki; Song, Liming; Al-Wardat, Mashhoor; Khasawneh, Awni \| 收藏 \| 浏览/下载：14/0 \| 提交时间：2020/03/10 binaries: X-rays stars: neutron stars: fundamental parameters accretion disks formation magnetic fields
	onthepossibilityofdiskfedformationinsupergianthighmassxraybinaries 期刊论文 OAI收割天文和天体物理学研究英文版, 2019, 卷号: 000, 期号: 001, 页码: 123 作者: Ali Taani; Shigeyuki Karino; Liming Song; Mashhoor AlWardat; Awni Khasawneh \| 收藏 \| 浏览/下载：16/0 \| 提交时间：2020/03/11
	A New Set of Parameters of High-Mass X-ray Binaries Found with their Cyclotron Lines 期刊论文 OAI收割 arXiv e-prints, 2018 作者: Zhang, Chengmin; Taani, Ali; Chaty, Sylvain; Karino, Shigeyuki; Song, Liming \| 收藏 \| 浏览/下载：74/0 \| 提交时间：2019/07/12 Astrophysics - High Energy Astrophysical Phenomena Abstract: We have derived new physical quantities for several High-Mass X-ray Binaries (HMXBs) with supergiant (SG) companions through their cyclotron lines. The parameters are: the terminal velocity of the wind, the mass loss rate of the donor, the effective temperature and the magnetic fields. These parameters influence significantly the improvement of the model of accretion. In spite of the variety of their observational properties, the corresponding magnetic field is around B ~ 10^12 G. This result can be constrained by the effects on stellar evolution. In addition, we have performed a segmentation in the parameter space of donors intended for several SG-HMXB listed in our sample set. The parameter space can be categorized into five regimes depending on the possibility of disk formation associated with accretion from the stellar wind. This can give a quantitative clarification of the observed variability and the properties of these objects. We show that, when these systems come into the direct accretion region, systems with corresponding parameters can emit X-rays.