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Model Calculations on the Large Scale Distribution of Bubbles in Galaxies
Published online by Cambridge University Press: 04 August 2017
Extract
One main characteristic of the ionized and neutral component of the interstellar medium in galaxies is the appearance of shells and bubbles in all sizes up to 1 kpc diameter (Hodge, 1974; Heiles, 1979). Between different galaxy types differences in size and radial distribution of these bubbles are observed as a function of galaxy type. The stochastic selfpropagating star formation model is able to simulate such distributions on a global galactic scale.
- Type
- II. Spiral Structure
- Information
- Symposium - International Astronomical Union , Volume 100: Internal Kinematics and Dynamics of Galaxies , 1983 , pp. 137 - 138
- Copyright
- Copyright © Reidel 1983