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The Methanol Multibeam Survey

Published online by Cambridge University Press:  01 March 2007

James A. Green
Affiliation:
Jodrell Bank Observatory, The University of Manchester;
R. J. Cohen
Affiliation:
Jodrell Bank Observatory, The University of Manchester;
J. L. Caswell
Affiliation:
Australia Telescope National Facility;
G. A. Fuller
Affiliation:
The University of Manchester;
K. Brooks
Affiliation:
Australia Telescope National Facility;
M. G. Burton
Affiliation:
University of New South Wales;
A. Chrysostomou
Affiliation:
University of Hertfordshire;
P. J. Diamond
Affiliation:
Jodrell Bank Observatory, The University of Manchester;
S. P. Ellingsen
Affiliation:
University of Tasmania;
M. D. Gray
Affiliation:
The University of Manchester;
M. G. Hoare
Affiliation:
University of Leeds;
M. R. W. Masheder
Affiliation:
Bristol University;
N. McClure-Griffiths
Affiliation:
Australia Telescope National Facility;
M. Pestalozzi
Affiliation:
University of Hertfordshire;
C. Phillips
Affiliation:
Australia Telescope National Facility;
L. Quinn
Affiliation:
Jodrell Bank Observatory, The University of Manchester;
M. A. Thompson
Affiliation:
University of Hertfordshire;
M. Voronkov
Affiliation:
Australia Telescope National Facility;
A. Walsh
Affiliation:
James Cook University
D. Ward-Thompson
Affiliation:
University of Cardiff;
D. Wong-McSweeney
Affiliation:
The University of Manchester;
J. A. Yates
Affiliation:
University College, London.
J. Cox
Affiliation:
University of Cardiff;
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Abstract

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A new 7-beam methanol multibeam receiver is being used to survey the Galaxy for newly forming massive stars, that are pinpointed by strong methanol maser emission at 6.668 GHz. The receiver, jointly constructed by Jodrell Bank Observatory (JBO) and the Australia Telescope National Facility (ATNF), was successfully commissioned at Parkes in January 2006. The Parkes-Jodrell survey of the Milky Way for methanol masers is two orders of magnitude faster than previous systematic surveys using 30-m class dishes, and is the first systematic survey of the entire Galactic plane. The first 53 days of observations with the Parkes telescope have yielded 518 methanol sources, of which 218 are new discoveries. We present the survey methodology as well as preliminary results and analysis.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Brand, J., & Blitz, L. 1993, A&A 275, 67Google Scholar
Condon, J. J., Broderick, J. J., & Seielstad, G. A. 1989, ApJ 97, 1064CrossRefGoogle Scholar
Dame, T. M., Hartmann, D., & Thaddeus, P. 2001, ApJ 547, 792CrossRefGoogle Scholar
Keto, E. 2003, ApJ 599, 1196CrossRefGoogle Scholar
Menten, K. M. 1991, ApJ (Letters) 380, L75CrossRefGoogle Scholar
Minier, V., Ellingsen, S. P., Norris, R. P., & Booth, R. S. 2003, A&A 403, 1095Google Scholar
Pestalozzi, M. R., Minier, V., & Booth, R. S. 2005, A&A 432, 737Google Scholar
Pandian, J. D., Goldsmith, P. F., & Deshpande, A. A. 2007, ApJ 656, 255CrossRefGoogle Scholar
Yorke, H. W. 2004, in: Jayawardhana, R., Burton, M. G., & Bourke, T. L. (ed.), Star-Formation at High Angular Resolution (IAU Symposium 221), p. 141Google Scholar