Evolution from Interstellar Cloud to Stars

Details Evolution from Interstellar Cloud to Stars Evolution from Interstellar Cloud to Stars

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000asthe..93..604t&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 93, No. 10, p. 604 - 615 (2000)

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The evolution of interstellar clouds to form stars is summarized from a theoretical point of view. The author compares two typical solutions by which the gravitational contraction of cloud is expressed (Larson-Penston vs. Shu solution). In particular, he pays attention to the differences in the evolutions of magentically super- and subcritical clouds. Finally the role of bipolar molecular outflows and optical jets are discussed.

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