H2CO and OH observations of a molecular cloud near RCW 36

Details H2CO and OH observations of a molecular cloud near RCW 36 H2CO and OH observations of a molecular cloud near RCW 36

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pasau...3..147w&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 11th, Clayton, Victoria, Australia, May 30-June 1, 1977.) Astronomic

Astronomy and Astrophysics

Astronomy

9

Absorption Spectra, Formaldehyde, Hydroxyl Emission, Molecular Absorption, Cosmic Dust, Electron Transitions, H Ii Regions, Hydrogen Ions, Radio Telescopes

Scientific paper

Transition line observations made with the 64 m Parkes radio telescope of H2CO and OH in the H II region of RCW 36 have revealed that this region, which is contained within a lane of dust, is associated with a dense, elongated molecular cloud. Attention is given to the absorption spectra of H2CO and OH, which provide an indication of the absorption velocities in the cloud.

Affiliated with

Also associated with

No associations

Rating

H2CO and OH observations of a molecular cloud near RCW 36 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 H2CO and OH observations of a molecular cloud near RCW 36, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and H2CO and OH observations of a molecular cloud near RCW 36 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1099150