Calculation of HCN emission in dark clouds

Details Calculation of HCN emission in dark clouds Calculation of HCN emission in dark clouds

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66..264l&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, Mar.-Apr. 1989, p. 264-274. In Russian.

Astronomy and Astrophysics

Astronomy

1

Dark Matter, Hydrocyanic Acid, Molecular Clouds, Radiation Transport, Computerized Simulation, Hyperfine Structure, Interstellar Gas, Monte Carlo Method

Scientific paper

Radiation-transfer simulations were carried out for HCN with the aim of explaining the anomalous relative intensities of the hyperfine components in the J = 1-0 transition observed in cold interstellar clouds. Monte Carlo calculations were carried out for a spherically symmetric cloud with density falling as n(r) varies as the inverse of r squared.

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