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Water maser follow-up of the Methanol Multi-Beam Survey.

Published online by Cambridge University Press:  24 July 2012

Anita Titmarsh ,
Simon Ellingsen ,
Shari Breen ,
James Caswell  and
Maxim Voronkov
Anita Titmarsh
Affiliation:
School of Mathematics and Physics, University of Tasmania, Private Bag 37, Hobart, Tasmania 7001, Australia email: Anita.Titmarsh@utas.edu.au CSIRO Astronomy and Space Science, PO Box 76, Epping, NSW 1710
Simon Ellingsen
Affiliation:
School of Mathematics and Physics, University of Tasmania, Private Bag 37, Hobart, Tasmania 7001, Australia email: Anita.Titmarsh@utas.edu.au
Shari Breen
Affiliation:
CSIRO Astronomy and Space Science, PO Box 76, Epping, NSW 1710
James Caswell
Affiliation:
CSIRO Astronomy and Space Science, PO Box 76, Epping, NSW 1710
Maxim Voronkov
Affiliation:
CSIRO Astronomy and Space Science, PO Box 76, Epping, NSW 1710
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Abstract

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The Australia Telescope Compact Array has been used to observe all the 603 6.7 GHz methanol masers detected in the Methanol Multi-Beam survey between l = 310° - 20°. To date we have measured positions with arcsecond accuracy for all the observations in the l = 6° - 20°.

Keywords

masersstars: formationradio lines: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S287: Cosmic Masers - from OH to H0 , January 2012 , pp. 275 - 279
Copyright
Copyright © International Astronomical Union 2012

References

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