Angular momentum loss in star formation.

Details Angular momentum loss in star formation. Angular momentum loss in star formation.

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esoc...33...89p&link_type=abstract

ESO Workshop on Low Mass Star Formation and Pre-Main Sequence Objects, p. 89 - 94

Physics

1

Interstellar Clouds: Star Formation, Interstellar Clouds: Collapse, Binaries: Star Formation

Scientific paper

The author discusses how the angular problem may be solved during the collapse of a rotating cloud core. He considers collapse to a disc and subsequent disc evolution, which yields a single star with the angular momentum being dispersed in a disc. And he considers collapse to form a binary (or multiple) star system in which most of the angular momentum ends up in orbital motion.

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