Convection as a source of viscosity for accretion disks of cataclysmic binaries

Details Convection as a source of viscosity for accretion disks of cataclysmic binaries Convection as a source of viscosity for accretion disks of cataclysmic binaries

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...223..979v&link_type=abstract

Astrophysical Journal, Part 1, vol. 223, Aug. 1, 1978, p. 979-981.

Astronomy and Astrophysics

Astrophysics

14

Binary Stars, Convective Flow, Disks (Shapes), Dwarf Stars, Novae, Stellar Mass Accretion, Angular Momentum, Astronomical Models, Stellar Evolution, Viscosity

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1978ApJ...223..979V

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