Fragmentation

Details Fragmentation Fragmentation

May 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974mmsai..45..397m&link_type=abstract

(Ministero della Pubblica Istruzione, CNR, and Universita di Trieste, European Regional Meeting in Astronomy, 2nd, Trieste, Ital

Astronomy and Astrophysics

Astronomy

Fragmentation, Hydrogen Clouds, Star Clusters, Stellar Evolution, Turbulence Effects, Astronomical Models, Condensation, Energy Distribution, Pressure Effects, Shock Waves, Stellar Gravitation, Temperature Effects, Thermal Energy

Scientific paper

A spherical gas cloud which has been brought to the verge of gravitational collapse by the pressure of the external medium is considered. An investigation is conducted of the possibility that during the collapse the cloud fragments into a large number of protostars. Attention is given to the effect of a galactic magnetic field and the model of a uniformly rotating cloud. Two extreme cases regarding the relation between magnetic field and angular velocity are studied.

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