A comparison of cloud formation rates in the gravitational instability and random collisional buildup models

Details A comparison of cloud formation rates in the gravitational instability and random collisional buildup models A comparison of cloud formation rates in the gravitational instability and random collisional buildup models

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...357..125e&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 357, July 1, 1990, p. 125-131.

Astronomy and Astrophysics

Astrophysics

16

Gravitational Effects, Molecular Clouds, Molecular Collisions, Monte Carlo Method, Star Formation, Interstellar Matter, Space Density, Taylor Instability

Scientific paper

The cloud collision time scale and the overall cloud formation time scale in the random collisional buildup model of molecular cloud formation are compared to the cloud formation time scale in the gravitational instability model. Observed values of the molecular cloud space density, gravitationally enhanced collision cross section, and velocity dispersion are used. Because the column density of a virialized cloud is proportional to the square root of the ambient pressure, the collision rate for molecular clouds depends only on the square root of the average interstellar density and is independent of velocity dispersion. This density dependence is the same for gravitational instabilities, so the ratio of cloud formation rates in the two models is independent of density and velocity dispersion. Two Monte Carlo simulations for random collisions are discussed. The results suggest that gravitational instabilities generally form large clouds faster than random collisions by a factor of about three.

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