Observations of the carbon star CIT 6 in the CO and HCN lines

Details Observations of the carbon star CIT 6 in the CO and HCN lines Observations of the carbon star CIT 6 in the CO and HCN lines

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..870z&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, July-Aug. 1987, p. 870-872. In Russian.

Astronomy and Astrophysics

Astrophysics

Carbon Monoxide, Carbon Stars, Hydrocyanic Acid, Line Spectra, Stellar Spectra, Stellar Spectrophotometry, Abundance, Emission Spectra, Molecular Spectra, Radio Spectra

Scientific paper

Emission from the carbon star CIT 6 in the J = 1-0 spectral lines of CO and HCN was observed with the Crimean Astrophysical Observatory RT-22 radio telescope during 1984-1985. Differences between the present spectra and those obtained earlier suggest that the molecular radio emission of CIT 6 may be variable. The angular dimension of the HCN emission region in CIT 6 is about 25 arcmin; the relative abundance of HCN molecules in the CIT 6 envelope is greater than about 10 to the -8th.

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