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The 44 GHz methanol maser line in massive star forming regions

Published online by Cambridge University Press:  01 March 2007

P. Hofner ,
E. Jordan ,
E. Araya  and
S. Kurtz
P. Hofner
Affiliation:
New Mexico Tech, NM, USA National Radio Astronomy Observatory, NM, USA
E. Jordan
Affiliation:
New Mexico Tech, NM, USA
E. Araya
Affiliation:
New Mexico Tech, NM, USA National Radio Astronomy Observatory, NM, USA
S. Kurtz
Affiliation:
Centro de Radioastronomía y Astrofísica, UNAM, Morelia, México email: phofner@nrao.edu
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Abstract

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We present the results of recent surveys in the 44GHz methanol maser line toward regions of massive star formation using the Haystack 37m telescope and the VLA. We discuss a possible shock origin of this maser line and present evidence for variability from multi-epoch observations of selected sources.

Keywords

maserssurveysISM:moleculesradio lines:ISMstars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S242: Astrophysical Masers and their Environments , March 2007 , pp. 160 - 161
Copyright
Copyright © International Astronomical Union 2008

References

Haschick, A. D., Menten, K., & Baan, W. A. 1990, ApJ 354, 556Google Scholar
Kurtz, S., Hofner, P. & Vargas-Alvarez, C. 2004, ApJS 155, 149CrossRefGoogle Scholar