Fission candidates among detached close binaries

Details Fission candidates among detached close binaries Fission candidates among detached close binaries

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..99...75o&link_type=abstract

(International Astronomical Union, Colloquium on Double Stars, Physical Properties and Generic Relations, 80th, Bandung, Indones

Astronomy and Astrophysics

Astrophysics

Binary Stars, Main Sequence Stars, Stellar Evolution, Stellar Motions, Stellar Rotation, Gravitational Collapse, Mass Ratios, Protostars, Stellar Mass

Scientific paper

A comparison between results of model calculations and observed properties of close, but detached low mass binaries with main sequence primaries shows statistical trends, which seem to support fission origin for some of these objects: the mass-momentum relation, the relation between mass ratio and separation and the relation between mass ratio and synchronisation speak in favour of close initial separations and small mass ratios of the components.

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