OH emission from Mira variables, infrared stars and molecular clouds

Details OH emission from Mira variables, infrared stars and molecular clouds OH emission from Mira variables, infrared stars and molecular clouds

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...59..465s&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 59, March 1985, p. 465-483.

Astronomy and Astrophysics

Astronomy

17

Hydroxyl Emission, Infrared Stars, Interstellar Masers, Mira Variables, Molecular Clouds, Radio Stars, Variable Stars, Linear Polarization, M Stars, Microwave Emission, Radiant Flux Density, Radio Sources (Astronomy), Stellar Spectra

Scientific paper

A sample of 79 stellar sources has been searched for the 18 cm wavelength OH lines. Seven of the eighteen newly detected OH sources have a stellar origin and the others probably originate from molecular clouds. Five sources were detected in other lines than previously known, and for a number of already known (stellar) OH masers new features were found. The 1612 MHz line of the Mira variable UX Cyg was found to be linearly polarized, though to a lesser extent than the main lines are.

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