Boundary layer theory and its application to Algol systems - A model for the pseudo-photosphere stars

Details Boundary layer theory and its application to Algol systems - A model for the pseudo-photosphere stars Boundary layer theory and its application to Algol systems - A model for the pseudo-photosphere stars

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...154..263s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 154, no. 1-2, Jan. 1986, p. 263-266.

Astronomy and Astrophysics

Astronomy

10

Accretion Disks, Binary Stars, Hydrodynamics, Stellar Mass Accretion, Stellar Models, Turbulent Boundary Layer, Late Stars, Main Sequence Stars, Stellar Atmospheres, Ultraviolet Astronomy

Scientific paper

Mass accretion onto main sequence stars in Algol systems must take place in a shear-dominated boundary layer. This study shows that many of the gross observational properties of these systems can be understood to arise from such regions, in which turbulent coupling to the underlying star is important. Specific systems are discussed, and comparison is also made to previous numerical hydrodynamic simulations.

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