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The Central Molecular Zone with Mopra

Published online by Cambridge University Press:  21 March 2013

Michael G. Burton  and
Paul A. Jones
Michael G. Burton
Affiliation:
School of Physics, University of New South Wales Sydney, NSW 2052, Australia
Paul A. Jones
Affiliation:
School of Physics, University of New South Wales Sydney, NSW 2052, Australia
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Abstract

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We outline a project to map the molecular line emission from the Central Molecular Zone across the 3–12 mm wavebands using the Mopra telescope in Australia. The dataset facilitates use of the CMZ as a template against which observations of molecular emission in other galactic nuclei may be interpreted.

Keywords

Galaxy: center — ISM: molecules
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. 75 - 78
Copyright
Copyright © International Astronomical Union 2013

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