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Turbulence and stochastic star formation in the Large Magellanic Cloud
Published online by Cambridge University Press: 19 July 2016
Abstract
A recent turbulence analysis of the Large Magellanic Cloud (LMC) is summarized. New model calculations on stochastic self-propagating star formation taking into account the multi-phase structure of the interstellar medium are presented. The relationship between star formation and turbulence is discussed.
- Type
- Large-Scale Structure and Kinematics
- Information
- Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 103 - 104
- Copyright
- Copyright © Kluwer 1991