Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-25T18:16:20.141Z Has data issue: false hasContentIssue false
  • English
  • Français

Exploring the Nature of MMB sources: A Search for Class I Methanol Masers and their Outflows

Published online by Cambridge University Press:  16 July 2018

Nichol Cunningham ,
Gary Fuller ,
Adam Avison  and
Shari Breen
Nichol Cunningham
Affiliation:
Green Bank Observatory, 155 Observatory Rd, P.O. Box 2, Green Bank, WV, 24944, USA email: [email protected]
Gary Fuller
Affiliation:
Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, UK
Adam Avison
Affiliation:
Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, UK
Shari Breen
Affiliation:
Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present the initial results from a class I 44-GHz methanol maser follow-up survey, observed with the MOPRA telescope, towards 272 sources from the Methanol Multi-beam survey (MMB). Over half (∼60%) of the 6.7 GHz class II MMB maser sources are associated with a class I 44-GHz methanol maser at a greater than 5σ detection level. We find that class II MMB masers sources with an associated class I methanol maser have stronger peak fluxes compared to regions without an associated class I maser. Furthermore, as part of the MOPRA follow-up observations we simultaneously observed SiO emission which is a known tracer of shocks and outflows in massive star forming regions. The presence of SiO emission, and potentially outflows, is found to be strongly associated with the detection of class I maser emission in these regions.

Keywords

masersstars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S336: Astrophysical Masers: Unlocking the Mysteries of the Universe , September 2017 , pp. 317 - 318
Copyright
Copyright © International Astronomical Union 2018 

References

Breen, S. L., Ellingsen, S. P., Caswell, J. L., & Lewis, B. E., 2010, MNRAS, 401, 2219Google Scholar
Cunningham, N., Lumsden, S. L., Cyganowski, C. J., et al., 2016, MNRAS, 458, 1742Google Scholar
Gibb, A. G., Davis, C. J., & Moore, T. J. T., 2007, MNRAS, 382, 1213CrossRefGoogle Scholar
Green, J. A., Caswell, J. L., Fuller, G. A., Avison, A., et al., 2009, MNRAS, 392, 783Google Scholar
Green, J. A. & McClure-Griffiths, N. M., 2011, MNRAS, 417, 2500Google Scholar
Jordan, C. H., Walsh, A. J., Breen, S. L., Ellingsen, S. P., et al., 2017, MNRAS, 471, 3915CrossRefGoogle Scholar
Klaassen, P. D., Testi, L., & Beuther, H., 2012, A&A, 583, A140Google Scholar
Leurini, S., Codella, C., López-Sepulcre, A., Gusdorf, A., et al., 2014, A&A, 570, A49Google Scholar