OH radio emission sources in W33

Details OH radio emission sources in W33 OH radio emission sources in W33

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..105p&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Feb. 1980, p. 105-109.) Soviet Astronomy Letters, vol. 6, Jan.-Feb. 1980, p. 58-60.

Astronomy and Astrophysics

Astronomy

1

Hydroxyl Emission, Interstellar Masers, Molecular Clouds, Radio Sources (Astronomy), Antennas, Circular Polarization, Line Spectra, Radial Velocity, Radio Telescopes

Scientific paper

The field of W33 was observed in the 18-cm OH lines with the Nancay
radio telescope in 1978. Dense molecular clouds as well as type IIc OH
emission sources have been detected near the type I OH masers W33A, B,
C, suggesting that type IIc OH emission sources represent such clouds.

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