Computer Science – Numerical Analysis
Scientific paper
May 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974mmsai..45..441w&link_type=abstract
(Ministero della Pubblica Istruzione, CNR, and Universita di Trieste, European Regional Meeting in Astronomy, 2nd, Trieste, Ital
Computer Science
Numerical Analysis
Angular Momentum, Condensation, Interstellar Gas, Star Formation, Gas Density, Numerical Analysis, Stellar Gravitation, Stellar Mass, Stellar Rotation
Scientific paper
Problems concerning the process of star formation are related to difficulties regarding the angular momentum and the absence of a correlation between the axis of stellar rotation and the rotation of the Galaxy. In an attempt to resolve these problems, it is supposed that star formation occurs by the accumulation of a large number of randomly moving subcondensations. An investigation is conducted concerning the general conditions which these subcondensations must satisfy if they are to play a part in the development of a gas cloud.
Donnison J. R.
Williams Iwan P.
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