Interstellar CH toward Zeta Ophiuchi

Details Interstellar CH toward Zeta Ophiuchi Interstellar CH toward Zeta Ophiuchi

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...326..905p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 326, March 15, 1988, p. 905-908.

Statistics

Computation

7

Abundance, Interstellar Matter, Methyl Compounds, Molecular Clouds, Ophiuchi Clouds, Signal To Noise Ratios, Absorption Spectra, Computational Astrophysics, Line Shape, Line Spectra

Scientific paper

Measurements of the equivalent width and the intrinsic width of two lines CH 3879 and CH 2886 in the direction of Zeta Ophiuchi are presented. The results indicate that the molecular line widths have a substantial thermal component. The temperature implied by the widths, about 1200 K, is much higher than those found from other diagnostic or found in any models of such clouds. A relation between the CH and CN molecular line widths in the Zeta Oph cloud is suggested.

Affiliated with

Also associated with

No associations

Rating

Interstellar CH toward Zeta Ophiuchi 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 Interstellar CH toward Zeta Ophiuchi, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interstellar CH toward Zeta Ophiuchi will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1671248