Discovery of an Intense OH Emission Source

Citations Over TimeTop 10% of 1969 papers

Abstract

Abstract : This letter reports the discovery of a bright OH emission source at 1612.231 MHz in the constellation Canis Major. The source was discovered with the Owens Valley interferometer in October, 1968. There is a bright infrared object listed close to the position of the source in the Caltech catalog of infrared stars (Neugebauer and Leighton 1968). This infrared object has been identified with an irregular variable, VY Canis Majoris. (Author)

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