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Periodic Orbits and Accretion Disks
Celestial Mechanics and Dynamical Astronomy, 1997The motion of a small particle in a binary system where the radiation pressure is not negligible is considered. The photogravitational three-body problem is used as a model of formation of a disc by accretion. The author generalizes the method of \textit{Paczyńsky} [Astrophys. J.
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Counterrotating Galaxies and Accretion Disks
Annals of the New York Academy of Sciences, 1998ABSTRACT:Theoretical interest in astrophysical disks with counterrotating components of stars and/or gas has been stimulated by recently discovered counterrotating spiral and S0 galaxies. A variety of physical processes can occur in counterrotating disks.
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Accretion Disk Electrodynamics
1987A plasma cloud orbiting around a compact object of mass M with the Kepler velocity vϕ = (GM/ r)1/2 at a distance r from the center of the object has an angular momentum I = mΩr2 , where m is the mass of the cloud and Ω = vϕ/r is tne angular velocity.
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Circumbinary Accretion: From Binary Stars to Massive Binary Black Holes
Annual Review of Astronomy and Astrophysics, 2023Dong Lai, Diego José Muñoz
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Accretion onto Pre-Main-Sequence Stars
Annual Review of Astronomy and Astrophysics, 2016Lee Hartmann +2 more
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Three-Layered Atmospheric Structure in Accretion Disks Around Stellar-Mass Black Holes
Science, 2000Shuang-Nan Zhang, Wei Cui
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