close binary
In a detached binary, neither star fills its Roche lobe, so that there is no significant mass transfer between the components. In a semidetached binary, one of the stars fills its Roche lobe, which results in this star losing material in a matter stream that either falls directly onto its companion, or, as is more usual, that enters an accretion disk. In a contact binary both components fill their Roche lobes or, more often, overflow them so that there is a common convective envelope. The proximity of stars in close binaries typically stretches at least one component into an ellipsoidal variable, and often produces an eclipsing binary as well. Related categories • TYPES OF STAR STELLAR ASTROPHYSICS Also on this site: Encyclopedia of Alternative Energy & Sustainable Living Encyclopedia of History Transport Concepts & Designs (partner site) |