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Molecular Gas and Dust in Nearby Galactic Centers: from SMA to ALMA
Published online by Cambridge University Press: 21 March 2013
Abstract
SMA observations of molecular gas and dust in nearby galactic centers are presented to showcase remarkable ISM properties including warm to very hot gas, molecular clouds producing massive star clusters, and mechanical feedback through bubbles and outflows.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 143 - 148
- Copyright
- Copyright © International Astronomical Union 2013