Modes of Mass Ejection by Binary Stars and the Effect on Their Orbital Periods.
- 1 August 1963
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 138, 471
- https://doi.org/10.1086/147659
Abstract
Three modes of mass ejection from one or both components of a binary system have been idealized and their physical characteristics discussed, in order to predict their effect on the orbital period of the system. Also, the consequence of synchronization of axial rotation of component stars with their orbital revolution is examined.Keywords
This publication has 0 references indexed in Scilit: