Detection of (C-13)O J = 3-2 in IC 342 - Warm, clumpy molecular gas

Details Detection of (C-13)O J = 3-2 in IC 342 - Warm, clumpy molecular gas Detection of (C-13)O J = 3-2 in IC 342 - Warm, clumpy molecular gas

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...361l..45w&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 361, Oct. 1, 1990, p. L45-L48.

Astronomy and Astrophysics

Astrophysics

40

Carbon Dioxide, Carbon 13, Interstellar Gas, Molecular Clouds, Molecular Spectra, Line Spectra, Molecular Gases

Scientific paper

The detection of the (C-13)O J = 3-2 line is reported, and a 15-arcsec-resolution, seven-point map of the (C-12)O J = 3-2 line in IC 342 is presented. The (C-13)O line strength, when compared to the lower-J line strengths at similar spatial resolution, suggests that the (C-13)O lines are optically thick in the inner 200 pc of IC 342. The physical conditions in the molecular gas in the inner region of IC 342 are similar to the conditions in the inner 200 pc of the Galaxy.

Affiliated with

Also associated with

No associations

Rating

Detection of (C-13)O J = 3-2 in IC 342 - Warm, clumpy molecular gas 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 Detection of (C-13)O J = 3-2 in IC 342 - Warm, clumpy molecular gas, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of (C-13)O J = 3-2 in IC 342 - Warm, clumpy molecular gas will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1302139