On the possible turbulence mechanism in accretion disks in nonmagnetic binary stars-Reference-Cited by-同舟云学术

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On the possible turbulence mechanism in accretion disks in nonmagnetic binary stars

Published:2014-08-31 Issue:8 Volume:57 Page:787-798
ISSN:1063-7869
Container-title:Physics-Uspekhi
language:
Short-container-title:Phys.-Usp.

Author:

Kurbatov E P,Bisikalo D V,Kaygorodov P V

Publisher

Uspekhi Fizicheskikh Nauk (UFN) Journal

Subject

General Physics and Astronomy

Link

http://stacks.iop.org/1063-7869/57/i=8/a=787/pdf

Cited by 13 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Gas-Dynamical Model of Accretion on a Neutron Star with Viscosity and the Influence of Large-Scale Vortices on the Transmission of Angular Momentum;Astronomy Reports;2024-05

2. Point-wise Self-similar Solution for Spiral Shocks in an Accretion Disk with Mass Outflow in a Binary;The Astrophysical Journal;2021-11-25

3. The role of atmospheric outflows in the migration of hot Jupiters;Monthly Notices of the Royal Astronomical Society;2021-07-15

4. Migration of Hot Jupiters Induced by Atmosphere Outflow;Astronomy Reports;2020-12

5. A review of the disc instability model for dwarf novae, soft X-ray transients and related objects;Advances in Space Research;2020-09

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