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How to Interpret the Bubble-Dominated ISM in the LMC?
Published online by Cambridge University Press: 25 May 2016
Abstract
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3D computer simulations are used to discuss shapes, expansion velocties, masses and fragmentation of expanding shells in the LMC.
- Type
- Part 2. Interstellar Medium
- Information
- Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 106 - 107
- Copyright
- Copyright © Astronomical Society of the Pacific 1999
References
Palouš, J.
1990, in The Interstellar Disk-Halo Connection in Galaxies, ed. Bloemen, H., Sterrewacht Leiden, p. 101
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