The detection of OH in the Large Magellanic Cloud

Details The detection of OH in the Large Magellanic Cloud The detection of OH in the Large Magellanic Cloud

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.176p..25w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 176, July 1976, p. 25P-27P.

Astronomy and Astrophysics

Astronomy

22

Absorption Spectroscopy, Hydroxyl Emission, Magellanic Clouds, Radio Astronomy, Carbon Monoxide, Emission Spectra, Formaldehyde, H Ii Regions, Molecular Spectra, Radial Velocity

Scientific paper

OH has been detected in absorption towards the compact H II region N159
in the Large Magellanic Cloud. The heliocentric velocity (253 km/s) and
half-intensity width (10 km/s) of the absorption profile are similar to
corresponding parameters for CO emission and H2CO absorption detected
previously.

Affiliated with

Also associated with

No associations

Rating

The detection of OH in the Large Magellanic Cloud 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 The detection of OH in the Large Magellanic Cloud, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The detection of OH in the Large Magellanic Cloud will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-940465