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Simulations on the Collisional Properties of Gas in Galaxies
Published online by Cambridge University Press: 26 May 2016
Abstract
In this work, we explore a simple method with few free parameters, which describes the global dynamical consequences on disk galaxies of a slow cycling of gas between the interstellar, almost collisionless very cold gas and the warm collisional phases, with a secular transformation of a fraction of warm gas into stars.
- Type
- Part 2. Origin
- Information
- Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 228 - 229
- Copyright
- Copyright © Astronomical Society of the Pacific 2004