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- W3102936594 abstract "Recent X-ray observations have revealed the complexity and diversity of high-mass X-ray binaries (HMXBs). This diversity challenges a classical understanding of the accretion process onto the compact objects. In this study, we reinforce the conventional concept of the nature of wind-fed accretion onto a neutron star considering the geometrical effect of radiatively accelerated wind, and re-evaluate the transported angular momentum by using a simple wind model. Our results suggest that even in an OB-type HMXB fed by stellar wind, a large amount of angular momentum could be transported to form an accretion disk due to the wind-inhomogeneity, if the binary separation is tight enough and/or stellar wind is slow. We apply our model into actual systems such as LMC X-4 and OAO 1657-415, and discuss the possibility of disk formations in these systems." @default.
- W3102936594 created "2020-11-23" @default.
- W3102936594 creator A5013979723 @default.
- W3102936594 creator A5043380454 @default.
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- W3102936594 date "2019-04-21" @default.
- W3102936594 modified "2023-10-03" @default.
- W3102936594 title "Stellar wind accretion and accretion disk formation: Applications to neutron star high-mass X-ray binaries" @default.
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- W3102936594 doi "https://doi.org/10.1093/pasj/psz034" @default.
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