Planetary systems as the ultimate or secondary product of binary star formation

Astronomy and Astrophysics – Astronomy

Scientific paper

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Binary Stars, Planetary Systems, Protostars, Star Formation, Extrasolar Planets, Star Distribution, Stellar Evolution, Stellar Rotation

Scientific paper

The distribution of spectral binaries as a function of the ratio of component masses is analyzed. A scheme is presented for the formation of a binary due to the rotational-exchange decay of a differentially rotating protostar. These results constitute a contribution to a new gasdynamic planetary cosmogony which views planets as the ultimate or secondary product of binary-star evolution, in contrast to conventional nebular hypotheses.

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