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The Australia Telescope campaign to study southern class I methanol masers

Published online by Cambridge University Press:  01 March 2007

M. A. Voronkov ,
K. J. Brooks ,
A. M. Sobolev ,
S. P. Ellingsen ,
A. B. Ostrovskii  and
J. L. Caswell
M. A. Voronkov
Affiliation:
Australia Telescope National Facility, PO Box 76, Epping, NSW 1710 email: [email protected]
K. J. Brooks
Affiliation:
Australia Telescope National Facility, PO Box 76, Epping, NSW 1710 email: [email protected]
A. M. Sobolev
Affiliation:
Ural State University, Lenin ave. 51, 620083 Ekaterinburg, Russia
S. P. Ellingsen
Affiliation:
University of Tasmania, GPO Box 252-37, Hobart, Tasmania 7000, Australia
A. B. Ostrovskii
Affiliation:
Ural State University, Lenin ave. 51, 620083 Ekaterinburg, Russia
J. L. Caswell
Affiliation:
Australia Telescope National Facility, PO Box 76, Epping, NSW 1710 email: [email protected]
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Abstract

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The Australia Telescope Compact Array (ATCA) and the Mopra facility have been used to search for new southern class I methanol masers at 9.9, 25(J=5) and 104 GHz, which are thought to trace more energetic conditions in the interface regions of molecular outflows, than the widespread class I masers at 44 and 95 GHz. One source shows a clear outflow association.

Keywords

Methanol masersoutflows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S242: Astrophysical Masers and their Environments , March 2007 , pp. 182 - 183
Copyright
Copyright © International Astronomical Union 2008

References

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