A strong 1665-MHz OH maser in the Large Magellanic Cloud

Details A strong 1665-MHz OH maser in the Large Magellanic Cloud A strong 1665-MHz OH maser in the Large Magellanic Cloud

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.197p..23h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 197, Dec. 1981, p. 23P-25P.

Astronomy and Astrophysics

Astronomy

18

Hydrogen Ions, Hydroxyl Emission, Interstellar Masers, Magellanic Clouds, Microwave Spectra, H Ii Regions, Luminous Intensity, Photoabsorption, Polarization Characteristics, Superhigh Frequencies

Scientific paper

A new OH Type I maser has been discovered in the Large Magellanic Cloud in the direction of the H II region N105. The 1665-MHz emission has a peak intensity of nearly 1 Jy and is strongly polarized in the right-hand circular sense. Weaker OH emission at 1667 MHz was also found but none at 1612 or 1720 MHz. No H2CO was detected in the direction of N105.

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