Physical connection between maser sources W75S and N

Details Physical connection between maser sources W75S and N Physical connection between maser sources W75S and N

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978azh....55...76l&link_type=abstract

Astronomicheskii Zhurnal, vol. 55, no. 1, 1978, p. 76-78. In Russian.

Astronomy and Astrophysics

Astronomy

Absorption Spectra, Hydroxyl Emission, Interstellar Masers, Radio Sources (Astronomy), H Ii Regions, Pdp 8 Computer, 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.

Affiliated with

Also associated with

No associations

Rating

Physical connection between maser sources W75S and N does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Physical connection between maser sources W75S and N, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physical connection between maser sources W75S and N will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1034632