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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

Kazushi Sakamoto
Kazushi Sakamoto*
Affiliation:
Academia Sinica, Institute of Astronomy and Astrophysics Taipei 10617, Taiwan email: ksakamoto@asiaa.sinica.edu.tw
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Abstract

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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.

Keywords

galaxies: ISM — galaxies: nuclei — galaxies: active
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

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