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37 GHz methanol masers: Horsemen of the apocalypse for the class II methanol maser phase?


Ellingsen, SP and Breen, SL and Sobolev, AM and Voronkov, MA and Caswell, JL and Lo, N, 37 GHz methanol masers: Horsemen of the apocalypse for the class II methanol maser phase?, The Astrophysical Journal: An International Review of Astronomy and Astronomical Physics, 742, (2) Article 109. ISSN 0004-637X (2011) [Refereed Article]

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Copyright 2011. The American Astronomical Society.

DOI: doi:10.1088/0004-637X/742/2/109


We report the results of a search for class II methanol masers at 37.7, 38.3, and 38.5 GHz toward a sample of 70 high-mass star formation regions. We primarily searched toward regions known to show emission either from the 107 GHz class II methanol maser transition, or from the 6.035 GHz excited OH transition. We detected maser emission from 13 sources in the 37.7 GHz transition, eight of these being new detections. We detected maser emission from three sources in the 38 GHz transitions, one of which is a new detection. We find that 37.7 GHz methanol masers are only associated with the most luminous 6.7 and 12.2 GHz methanol maser sources, which in turn are hypothesized to be the oldest class II methanol sources. We suggest that the 37.7 GHz methanol masers are associated with a brief evolutionary phase (of 1000-4000 years) prior to the cessation of class II methanol maser activity in the associated high-mass star formation region.

Item Details

Item Type:Refereed Article
Keywords:ISM: molecules - masers - radio lines: ISM - stars: formation
Research Division:Physical Sciences
Research Group:Astronomical sciences
Research Field:Galactic astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding knowledge
Objective Field:Expanding knowledge in the physical sciences
UTAS Author:Ellingsen, SP (Professor Simon Ellingsen)
UTAS Author:Breen, SL (Dr Shari Breen)
ID Code:74278
Year Published:2011
Web of Science® Times Cited:26
Deposited By:Mathematics and Physics
Deposited On:2011-11-17
Last Modified:2017-11-03

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