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Imaging of selected sources from the Methanol Multibeam Survey

Published online by Cambridge University Press:  01 March 2007

D. Wong-McSweeney ,
G. A. Fuller  and
S. Etoka
D. Wong-McSweeney
Affiliation:
School of Physics and Astronomy, University of Manchester, Sackville Street Building, Sackville Street, PO Box 88, Manchester, M60 1QD email: d.wong-mcsweeney@postgrad.manchester.ac.uk
G. A. Fuller
Affiliation:
School of Physics and Astronomy, University of Manchester, Sackville Street Building, Sackville Street, PO Box 88, Manchester, M60 1QD email: d.wong-mcsweeney@postgrad.manchester.ac.uk
S. Etoka
Affiliation:
School of Physics and Astronomy, University of Manchester, Sackville Street Building, Sackville Street, PO Box 88, Manchester, M60 1QD email: d.wong-mcsweeney@postgrad.manchester.ac.uk
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Abstract

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High angular resolution observations are essential for understanding the nature of maser emission and the sources which excite it. Here we present preliminary results from MERLIN observations of three methanol masers from the Toruń survey. These MERLIN observations are being analysed as part of the interferometric component of the Methanol Multibeam (MMB) Survey which is surveying the Galactic plane at |b|≤2° for 6.67 GHz methanol maser sources.

Keywords

maserssurveysstars: formationISM: individual (G20.24+0.07, G22.45-0.17, G23.01-0.41) galaxies: individual (Milky Way)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S242: Astrophysical Masers and their Environments , March 2007 , pp. 184 - 185
Copyright
Copyright © International Astronomical Union 2008

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