Methanol Maser Emission in W75N and Orion Molecular Cloud 2 (OMC 2)

Details Methanol Maser Emission in W75N and Orion Molecular Cloud 2 (OMC 2) Methanol Maser Emission in W75N and Orion Molecular Cloud 2 (OMC 2)

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...199.0413g&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #04.13; Bulletin of the American Astronomical Society, Vol. 33, p.1308

Astronomy and Astrophysics

Astronomy

Scientific paper

We present data of Class I methanol maser emission at 44 GHz centered on two star forming regions, W75N and Orion Molecular Cloud 2 (OMC 2). The Northeast Radio Observatory Corporation (NEROC) Haystack 37-m radio telescope was used to search for emission in the 70 to 61 A+ transition of CH3OH as part of a larger project lead by Dr. Preethi Pratap (MIT Haystack Observatory). This project focuses on detecting maser activity in positions that are offset from known young stellar objects. In addition to detecting the known methanol maser source in each region, a previously undetected maser source was observed to the southwest of W75N IRAS 1.

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