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1D, 2D and 3D Collapse of Interstellar Clouds

Published online by Cambridge University Press:  12 April 2016

W.M. Tscharnuter
W.M. Tscharnuter*
Affiliation:
Max Planck Institut für Astrophysik, Garching b. München, FRG

Extract

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This review is concerned with recent theoretical investigations and numerical models of star formation with varions symmetries. Observations strongly support the fact that stars condense out of cool (≈10 K) and dense (103-104 atoms/cm3) interstellar clouds due to gravitational instability and collapse. Bright, young stellar objects (0- and B-stars are always found in the vicinity of coloud complexes.

Type
I. ID, 2D, and 3D Collapse of Interstellar Clouds
Information
International Astronomical Union Colloquium , Volume 58: Stellar Hydrodynamics , August 1980 , pp. 235 - 246
Copyright
Copyright © Reidel 1980

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