Mapping observations of sulfur-containing carbon-chain molecules in Taurus Molecular Cloud 1 (TMC-1)

Details Mapping observations of sulfur-containing carbon-chain molecules in Taurus Molecular Cloud 1 (TMC-1) Mapping observations of sulfur-containing carbon-chain molecules in Taurus Molecular Cloud 1 (TMC-1)

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...394..539h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 394, no. 2, Aug. 1, 1992, p. 539-551. Research supported by Japan Society f

Astronomy and Astrophysics

Astrophysics

110

Astronomical Maps, Carbon, Dark Matter, Molecular Clouds, Brightness Distribution, Interstellar Chemistry, Interstellar Matter, Molecular Chains, Sulfur, Taurus Constellation

Scientific paper

High-resolution mapping observations of TMC-1 using the lines of CCS, C3S, C(S-32), and C(S-34) molecules are reported. The source was also observed at HC3N, HC5N, NH3, C4H, and HCS(+) lines with high signal resolution for a systematic comparison with sulfur-containing carbon-chain molecules. Accurate molecular distributions are derived, and the origin of chemical differences in TMC-1 are discussed with reference to recent observations of dark cloud cores and chemical model calculations.

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