Dynamical contraction of infinite plane-symmetric gas clouds

Details Dynamical contraction of infinite plane-symmetric gas clouds Dynamical contraction of infinite plane-symmetric gas clouds

Jul 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974pthph..52..147k&link_type=abstract

Progress of Theoretical Physics, vol. 52, July 1974, p. 147-160.

Physics

1

Cloud Physics, Contraction, Gravitational Collapse, Interstellar Gas, Stellar Evolution, Cosmology, Entropy, Equations Of Motion, Gas Dynamics, Ideal Gas, Protostars, Solar System

Scientific paper

An investigation is conducted of the collapse of flat gas clouds. The assumption is made that the motion of the gas is restricted to the direction parallel to the rotation axis. It is also assumed that the density varies only in the direction perpendicular to the plane. The configuration at gravitational equilibrium is studied along with the conditions of dynamical stability in the case of infinite plane-symmetric cloud, taking into account also a comparison with a spherically symmetric cloud.

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