OH emission in the direction of TV GEM and BI CYG

Details OH emission in the direction of TV GEM and BI CYG OH emission in the direction of TV GEM and BI CYG

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86.1926b&link_type=abstract

Astronomical Journal, vol. 86, Dec. 1981, p. 1926-1929.

Astronomy and Astrophysics

Astronomy

4

Hydroxyl Emission, Late Stars, M Stars, Stellar Spectra, Supergiant Stars, Infrared Astronomy, Iue, Line Spectra, Radio Sources (Astronomy)

Scientific paper

The NRAO-Green Bank 43-m telescope and 18-cm receiver have detected OH maser main-line emission at 1665 MHz, in the direction of the two late-type supergiants TV Gem and BI Cyg. The detection of the two new OH maser sources is noteworthy in view of the small number of late-type supergiants known to be molecular radio sources, or associated in close proximity with OH emission clouds. The IR, UV and radio properties of the two stars are discussed.

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