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UFN, 2008, Volume 178, Number 6, Pages 577–604 (Mi ufn603)  

This article is cited in 29 scientific papers (total in 29 papers)

REVIEWS OF TOPICAL PROBLEMS

The nature of accretion disks of close binary stars: overreflection instability and developed turbulence

A. M. Fridmanab, D. V. Bisikalob

a Russian Research Centre "Kurchatov Institute", Institute of Physics of Stochastic Structures
b Institute of Astronomy of the Russian Academy of Sciences

Abstract: The current status of the physics of accretion disks in close binary stars is reviewed, with an emphasis on the hydrodynamic overreflection instability, which is a factor leading to the accretion disk turbulence. The estimated turbulent viscosity coefficients are in good agreement with observations and explain the high angular momentum transfer rate and the measured accretion rate. Based on the observations, a power-law spectrum for the developed turbulence is obtained.

DOI: https://doi.org/10.3367/UFNr.0178.200806b.0577

Full text: PDF file (5976 kB)
Full text: http://www.ufn.ru/ru/articles/2008/6/b/
References: PDF file   HTML file

English version:
Physics–Uspekhi, 2008, 51:6, 551–576

Bibliographic databases:

PACS: 47.27.-i, 97.10.Gz, 97.80.-d
Received: February 28, 2008

Citation: A. M. Fridman, D. V. Bisikalo, “The nature of accretion disks of close binary stars: overreflection instability and developed turbulence”, UFN, 178:6 (2008), 577–604; Phys. Usp., 51:6 (2008), 551–576

Citation in format AMSBIB
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\paper The nature of accretion disks of close binary stars: overreflection instability and developed turbulence
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    Citing articles on Google Scholar: Russian citations, English citations
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    This publication is cited in the following articles:
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    2. Mikhailovskii A.B., Fridman A.M., Churikov A.P., Pustovitov V.D., Smolyakov A.I., “Ideal instabilities in a high-$\beta$ rotating cylindrical plasma in the presence of an azimuthal magnetic field and a gravitational field”, Plasma Phys. Control. Fusion, 51:4 (2009), 045003, 21 pp.  crossref  mathscinet  adsnasa  isi  elib  scopus
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    4. Kolesnichenko A.V., Marov M.Ya., “Magnetohydrodynamic simulation of the protoplanetary disk of the Sun”, Sol. Syst. Res., 43:5 (2009), 410–433  crossref  adsnasa  isi  elib  scopus
    5. Grinin V.P., Arkharov A.A., Barsunova O.Yu., Sergeev S.G., “Detection of low-amplitude brightness oscillations in the unique eclipsing system V718 Per (HMW 15, H 187)”, Astron. Lett., 35:12 (2009), 828–835  crossref  adsnasa  isi  elib  scopus
    6. Mishonov T.M., Dimitrov Z.D., Maneva Y.G., Hristov T.S., “Amplification of Slow Magnetosonic Waves by Shear Flow: Heating and Friction Mechanisms of Accretion Disks”, Space Plasma Physics, AIP Conference Proceedings, 1121, 2009, 28–54  crossref  adsnasa  isi  scopus
    7. A. G. Zhilkin, D. V. Bisikalo, “Formation of accretion disks in close-binary systems with magnetic fields”, Astron. Rep, 54:12 (2010), 1063  crossref  adsnasa  isi  elib  scopus
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    19. A. V. Kolesnichenko, “K modelirovaniyu szhimaemoi magnitogidrodinamicheskoi turbulentnosti akkretsionnogo protoplanetnogo diska”, Preprinty IPM im. M. V. Keldysha, 2014, 066, 47 pp.  mathnet
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