Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...160..181c&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 160, no. 1, May 1986, p. 181-184.
Astronomy and Astrophysics
Astrophysics
10
Abundance, Cyano Compounds, Molecular Clouds, Taurus Constellation, Cyanoacetylene, Interstellar Chemistry
Scientific paper
The authors report the detection of the J = 17-16 line of HC7N towards six cloudlets of the Taurus dark clouds complex. The HC7N column densities towards these globules range between 0.8x1012 and 4x1012cm-2, i.e., 4 - 20 times lower than towards TMC1. However, the average column density ratio N(HC5N)/N(HC7N) is 3.6, i.e., similar to the TMC1 one. Little variations of this abundance ratio are found from cloud to cloud whatever the total cyanopolyyne column density is. One of these cloudlets, L1495, is a new cyanopolyyne source and physical conditions towards it are derived from NH3, HC3N, and HC5N observations.
Bachiller Rafael
Cernicharo Jose
Duvert Gilles
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