The physical connection of the maser sources W75N and W75S

Details The physical connection of the maser sources W75N and W75S The physical connection of the maser sources W75N and W75S

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978sva....22...42l&link_type=abstract

(Astronomicheskii Zhurnal, vol. 55, no. 1, 1978, p. 76-78.) Soviet Astronomy, vol. 22, Jan.-Feb. 1978, p. 42, 43. Translation.

Astronomy and Astrophysics

Astronomy

Absorption Spectra, Hydroxyl Emission, Interstellar Masers, Radio Sources (Astronomy), Circular Polarization, Hydrogen Clouds, Radial Velocity, Superheterodyne Receivers

Scientific paper

The detection of new features in the 1667-MHz line profile of the maser source W75N is reported. An absorption line originating in a cold hydroxyl cloud on the background of a compact H II region near W75N was observed at a radial velocity of -3.5 km/sec. It is shown that the two compact H II regions (H II W75N and DR21) and the maser sources W75N and S are immersed in the same cold hydroxyl cloud. Variability in some of the OH emission features of W75N was recorded.

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