CO emission in directions of some millimeter wavelength continuum sources

Details CO emission in directions of some millimeter wavelength continuum sources CO emission in directions of some millimeter wavelength continuum sources

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...265..766k&link_type=abstract

Astrophysical Journal, Part 1, vol. 265, Feb. 15, 1983, p. 766-777.

Astronomy and Astrophysics

Astrophysics

7

Carbon Monoxide, Interstellar Matter, Millimeter Waves, Molecular Clouds, Continuous Radiation, Emission Spectra, Line Spectra, Spectrum Analysis, Velocity Distribution

Scientific paper

Observations of emission at 22.6 mm from 12CO, 13CO, and C18O from the nearby dark clouds L255, L673, L1471, and L1613 permit calculations of their molecular column densities for both CO and H2. Two of these clouds, L1613 and L673, are known to emit continuum radiation at millimeter wavelengths - presumably from embedded heated dust grains. The continuum emission correlates with the spatial distribution of the molecular column densities.

Affiliated with

Also associated with

No associations

Rating

CO emission in directions of some millimeter wavelength continuum sources 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 CO emission in directions of some millimeter wavelength continuum sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CO emission in directions of some millimeter wavelength continuum sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1305842