Classical Algol systems (Invited review)

Details Classical Algol systems (Invited review) Classical Algol systems (Invited review)

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..241b&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Physics

6

Eclipsing Binary Stars, Stellar Evolution, Stellar Physics, Variable Stars, Stellar Mass Accretion, Stellar Models

Scientific paper

Progress in the study of Algol-type binaries is presented in the light of more general efforts at compilation and categorization, some specific new and important observational results. Results can be referred to the well known underlying model of the semi-detached configuration and Roche lobe overflow mechanism. Successes and limitations of this model will be considered. Arising from such comparisons, lines of future research are suggested. Some outstanding issues concern: (1) the evolutionary condition of the mass accreting component, (2) instabilities and related effects in various regions of the flow, (3) systematic outflow, and (4) the relationship of classical Algols to other evolved binaries.

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