Star formation and contraction/fragmentation problems

Details Star formation and contraction/fragmentation problems Star formation and contraction/fragmentation problems

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hrgc.conf..209w&link_type=abstract

H II regions and the galactic centre : proceedings of the Eighth ESLAB Symposium, 4-7 June 1974, Frascati, Italy, p. 209-220 (SE

Computer Science

Contraction, Fragmentation, Stars, Stellar Evolution, Clouds, Condensing

Scientific paper

The processes that determine the mass spectrum and spatial configuration of stars formed in association are discussed, the processes are evaluated in terms of the energy imbalance which drives them and the competitivity of their time scale. A trend in the contraction/fragmentation sequence is outlined. This trend derives from the interaction between magnetic and centrifugal forces. The condensation time scale problem is considered.

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