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MALT90: tracing the chemistry and kinematics of molecular clumps within the central molecular zone

Published online by Cambridge University Press:  22 May 2014

Y. Contreras
Affiliation:
CSIRO Astronomy and Space Science PO Box 76, Epping 2122, Sydney, Australia email: [email protected]
J. Rathborne
Affiliation:
CSIRO Astronomy and Space Science PO Box 76, Epping 2122, Sydney, Australia email: [email protected]
J. Jackson
Affiliation:
Institute for Astrophysical Research, Boston University Boston, MA 02215, USA
J. Foster
Affiliation:
Yale Center for Astronomy and Astrophysics, Yale University New Haven, CT 06520, USA
S. Longmore
Affiliation:
Astrophysics Research Institute, Liverpool John Moore University Twelve Quays House, Egerton Wharf, Birkenhead CH 41 1LD, UK
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Abstract

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The MALT90 survey targets more than 2000 high-mass star-forming clumps in the Galactic plane obtaining small maps around each of them, in 16 molecular lines at 90 GHz. By observing several thousand high-mass star forming clumps MALT90 aims to characterize their global chemical and physical evolution. Here we summarize the survey parameters and show examples of the MALT90 data toward three clumps in the central molecular zone.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

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