Slow mass transfer in semidetached binaries

It is shown that, if the usual assumption of synchronous rotation (infinitely effective tidal coupling) in semidetached binary systems is replaced by that of detailed conservation of angular momentum with negligible tidal torques, the system is predicted to evolve in a qualitatively different manner...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astrophys. J., Lett., v. 204, no. 1, pp. L29-L33 Lett., v. 204, no. 1, pp. L29-L33, 1976-02, Vol.204, p.L29
Hauptverfasser:	Pratt, J. P., Strittmatter, P. A.
Format:	Artikel
Sprache:	eng
Schlagworte:	640102 -Physics Research-Astrophysics & Cosmology-Stars ANGULAR MOMENTUM BINARY STARS- ROTATION COSMIC X-RAY SOURCES HERTZSPRUNG-RUSSELL DIAGRAM N56200 -Physics (Astrophysics & Cosmology)-Stars N56300 -Physics (Astrophysics & Cosmology)-Quasi-stellar, Radio & X-Ray Sources STAR EVOLUTION
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