Structure of three molecular clouds from HC3N radio-line observations

Details Structure of three molecular clouds from HC3N radio-line observations Structure of three molecular clouds from HC3N radio-line observations

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..903k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, Dec. 1986, p. 903-911) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, Nov.-Dec

Astronomy and Astrophysics

Astronomy

2

Cyanoacetylene, Line Spectra, Molecular Clouds, Radio Astronomy, Abundance, Density Distribution, Hydrogen Clouds, Radial Velocity

Scientific paper

The intensity distribution of the line J = 4→3 HC3N was
measured in TMC-1, DR-21, M17. Models of these sources were constructed,
the distribution of the density was obtained. It was found that there
are clumps in these molecular clouds and it is in the clumps that star
formation occurs.

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