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pro vyhledávání: '"Ye, Yong‐Chun"'
Akademický článek
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Autor:
Tian, Yu, Qian, Xiao-Yan, Qin, Chao-Chao, Cui, Ming-Huan, Li, Yan-Qing, Ye, Yong-Chun, Wang, Jing-Kun, Wang, Wen-Jun, Tang, Jian-Xin
Publikováno v:
In Chemical Engineering Journal 1 July 2021 415
A model for 3:2 high-frequency quasi-periodic oscillations (HFQPOs) with 3:2 pairs observed in four black hole X-ray binaries (BHXBs) is proposed by invoking the epicyclic resonances with the magnetic connection (MC) between a spinning black hole (BH
Externí odkaz:
http://arxiv.org/abs/1601.07008
A magnetic model for low/hard state (LHS) of black hole X-ray binaries (BHXBs),H1743-322 and GX 339-4, is proposed based on the transportation of magnetic field from a companion into an accretion disk around a black hole (BH). This model consists of
Externí odkaz:
http://arxiv.org/abs/1508.07108
Akademický článek
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Three energy mechanisms invoking large-scale magnetic fields are incorporated in a model to interpret jet production in black hole (BH) systems, i.e., the Blandford-Znajek (BZ), the magnetic coupling (MC) and Blandford-Payne (BP) processes. These ene
Externí odkaz:
http://arxiv.org/abs/0711.4408
Publikováno v:
NewAstron.12:471-478,2007
A model of magnetic coupling (MC) of a rotating black hole (BH) with advection- dominated accretion flow (MCADAF) is proposed. It turns out that MCADAF providers a natural explanation for the transition radius between ADAF and SSD, and could be used
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701802
Publikováno v:
Astrophys.J.657:428-435,2007
We argue, following our earlier works (the "CEBZMC model"), that the phenomenon of twin peak high frequency quasi-periodic oscillations (QPOs) observed in black hole X-ray binaries is caused by magnetic coupling (MC) between accretion disk and black
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611592
Publikováno v:
Mon.Not.Roy.Astron.Soc.374:647-656,2007
A toy model for magnetic connection in black hole (BH) accretion disc is discussed based on a poloidal magnetic field generated by a single electric current flowing around a Kerr black hole in the equatorial plane. We discuss the effects of the coexi
Externí odkaz:
http://arxiv.org/abs/astro-ph/0603300
Publikováno v:
ApJ(2006), 643, 1047
A toy model for gamma-ray burst supernovae (GRB-SNe) is discussed by considering the effects of screw instability of magnetic field in black hole (BH) magnetosphere. The screw instability in the Blandford-Znajek (BZ) process (henceforth SIBZ) can coe
Externí odkaz:
http://arxiv.org/abs/astro-ph/0601707