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Galactic and extragalactic giant molecular clouds and massive star clusters: counting and analysis
Published online by Cambridge University Press: 31 March 2017
Abstract
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Comparative analysis of GMS and MSC is presented based on data collected on these objects in the Galaxy and other galaxies. The model is proposed of gravitational instability of GMC and MSC system. Some implications are discussed.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 12 , Symposium S316: Formation, evolution, and survival of massive star clusters , August 2015 , pp. 145 - 146
- Copyright
- Copyright © International Astronomical Union 2017
References
Grabelsky, D. A., Cohen, R. S., Bronfman, L., & Thaddeus, P.
1988, ApJ, 331, 181
CrossRefGoogle Scholar
Bronfman, L., Nyman, L., & Thaddeus, P.
1989, in: Winnewisser, G. & Armstrong, J. T. (eds.), The Physics and Chemistry of Interstellar Molecular Clouds - mm and Sub-mm Observations in Astrophysics, Lecture Notes in Physics (Berlin: Springer Verlag), 331, 139
Google Scholar
Draine, B. T.
2011, Physics of the Interstellar and Intergalactic Medium (Princeton University Press), 540
Google Scholar
Engargiola, G., Plambeck, R. L., Rosolowsky, E. & Blitz, L.
2001, ApJS, 149, 343
CrossRefGoogle Scholar
Bolatto, A. D., Leroy, A. K., Rosolowsky, E., Walter, F. & Blitz, L.
2008, ApJ, 686, 948
CrossRefGoogle Scholar
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