6.7 GHz Methanol Masers Associated with IRAS-Selected Sources

Details 6.7 GHz Methanol Masers Associated with IRAS-Selected Sources 6.7 GHz Methanol Masers Associated with IRAS-Selected Sources

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aj....116.2936m&link_type=abstract

The Astronomical Journal, Volume 116, Issue 6, pp. 2936-2942.

Astronomy and Astrophysics

Astronomy

29

Ism: H Ii Regions, Ism: Masers, Stars: Formation

Scientific paper

New detections of eight 6.7 GHz methanol masers have been made toward three samples of IRAS-selected objects. Two of the methanol maser sources have associated 1.6 GHz hydroxyl masers, and one has an associated 12.2 GHz methanol maser. The detection rate of the methanol masers is strongly dependent upon the IRAS colors of the sources. This dependence may arise from the conditions required for masing and reflect evolutionary changes in the star-forming regions. The reddest IRAS sources are the youngest.

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