Observations and analyses of interstellar Cyanogen

Details Observations and analyses of interstellar Cyanogen Observations and analyses of interstellar Cyanogen

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...240..811c&link_type=abstract

Astrophysical Journal, Part 1, vol. 240, Sept. 15, 1980, p. 811-827.

Astronomy and Astrophysics

Astrophysics

20

Cyanogen, Interstellar Gas, Molecular Spectra, Nebulae, Abundance, Astronomical Catalogs, Cyanoacetylene, Gas Density, H Ii Regions, Molecular Collisions

Scientific paper

CN was detected at 2 locations in the Taurus dark cloud complex and in 12 molecular clouds in H II regions; partial maps of CN line intensities were drawn for DR 21 and Sgr A. The line opacities and excitation temperatures were used to derive CN column densities in the ground rotational state. It was shown that: (1) CN is about as abundant as CS in molecular clouds associated with the H II regions, (2) opacities in the one to zero range of N lines of CN are small relative to unity, (3) CN is spatially correlated with NH3 and anticorrelated with HC3N in Taurus, and (4) in DR 21, CN is distributed similarly to HCN and C2H.

Affiliated with

Also associated with

No associations

Rating

Observations and analyses of interstellar Cyanogen 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 Observations and analyses of interstellar Cyanogen, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations and analyses of interstellar Cyanogen will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-904387