Computer Science – Numerical Analysis
Scientific paper
Sep 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993basi...21..597c&link_type=abstract
Astronomical Society of India, Bulletin (ISSN 0304-9523), vol. 21, no. 3-4, p. 597-600
Computer Science
Numerical Analysis
1
Angular Momentum, Dynamic Stability, Eclipsing Binary Stars, Mass Transfer, Orbit Perturbation, Ephemerides, Light Curve, Numerical Analysis
Scientific paper
The average mass transfer rates in four Algol-type binary stars RZ Cas, TV Cas, SW Cyg and DI Peg are derived from their observed period changes in the light of alternate period change model. The results have been used to discuss the anomalies in the mass transfer theory, namely dynamical instability of the mass losing component and the conservation of orbital angular momentum during the mass transfer.
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