Further observations of the N = 1-0 transition of C4H

Details Further observations of the N = 1-0 transition of C4H Further observations of the N = 1-0 transition of C4H

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...127..241b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 127, no. 1, Oct. 1983, p. 241-243.

Astronomy and Astrophysics

Astronomy

6

Hydrocarbons, Hyperfine Structure, Interstellar Matter, Molecular Clouds, Radio Sources (Astronomy), Free Radicals, Molecular Chains, Molecular Spectra

Scientific paper

High-sensitivity observations of the dust cloud TMC1 are presented for
all the hyperfine components of the N = 1-0 transition of C4H at 9.5
GHz. The results are shown and used to obtain an improved value of 1.3 x
10 to the 15th/sq cm for the densest part of TMC1. This value is about
four times greater than that given by Guelin et al. (1982).

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