Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.7107v&link_type=abstract
American Astronomical Society, 193rd AAS Meeting, #71.07; Bulletin of the American Astronomical Society, Vol. 30, p.1356
Astronomy and Astrophysics
Astronomy
1
Scientific paper
The cold, dark cloud cores are the important sites to probe the interstellar chemistry prevailing prior to the onset of collapse. TMC1 is an ideal object to study the chemistry in dark clouds under quiescent conditions. It shows a carbon rich chemistry with chemical gradients across its densest ridge extending over 0.2 pc x 0.6 pc. We present the results of the DSN 70m observations of complex carbon chain mol ecules (cumelene carbenes H_2C_n, radicals C_nH, cyanopolyynes HC_{2n+1}N, cumulene rings C_nH_2) at a few locations (CCS, cyanopolyyne, ammonia and SO peaks) along TMC1 ridge. We report the first detection of C_8H in TMC. Large differences are seen in t he intensity ratios among these molecules at different velocities as well as po sitions. Our results indicate differences in the chemical evolutionary statu s among the clumps in the TMC1 ridge. This can be interpreted in terms of a de nsity and time dependent chemical models for the formation and evolution of co mplex molecules. This research was conducted at the Jet Propulsion Laboratory, California Institute of Technology under support from the National Aeronautics and Space Administration.
Langer William D.
Velusamy Thangasamy
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