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

Journal Article · Sun Jul 01 04:00:00 EDT 1990 · Astrophysical Journal; (USA)

DOI:https://doi.org/10.1086/168897· OSTI ID:6863361

Elmegreen, B G ^[1]

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1. IBM Thomas J. Watson Research Center, Yorktown Heights, NY (USA)

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. 35 refs.

• OSTI ID: 6863361
• Journal Information: Astrophysical Journal; (USA), Journal Name: Astrophysical Journal; (USA) Vol. 357; ISSN ASJOA; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

640105* -- Astrophysics & Cosmology-- Galaxies
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COLLISIONS
COMPARATIVE EVALUATIONS
COSMIC GASES
DENSITY
FLUIDS
GASES
GRAVITATION
GRAVITATIONAL INSTABILITY
INSTABILITY
INTERSTELLAR SPACE
MATHEMATICAL MODELS
MOLECULE COLLISIONS
MONTE CARLO METHOD
PHYSICAL PROPERTIES
PLASMA INSTABILITY
SPACE
STAR EVOLUTION