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OH Emission in the Direction of TV Gem and BI Cyg
- Source :
- Mathematics, Physics, and Computer Science Faculty Articles and Research
- Publication Year :
- 1981
-
Abstract
- OH maser main-line emission at 1665 MHz has been detected in the direction of two late-type supergiants, TV Gem (Mllab) and BI Cyg (M3Iab), with the 43-m telescope and 18-cm receiver at NRAO-Green Bank. Detection of two new OH maser sources here is particularly interesting in view of the relatively small number of late-type supergiants that are known as molecular radio sources or associated in close proximity with OH emission clouds. The infrared, ultraviolet, and radio properties of these stars are discussed briefly.
Details
- Database :
- OAIster
- Journal :
- Mathematics, Physics, and Computer Science Faculty Articles and Research
- Notes :
- application/pdf
- Publication Type :
- Electronic Resource
- Accession number :
- edsoai.ocn894607817
- Document Type :
- Electronic Resource