Distribution of molecules in the vicinity of young B stars

Details Distribution of molecules in the vicinity of young B stars Distribution of molecules in the vicinity of young B stars

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..509r&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Aug. 1980, p. 509-512.) Soviet Astronomy Letters, vol. 6, July-Aug. 1980, p. 281-283

Astronomy and Astrophysics

Astronomy

Abundance, B Stars, Early Stars, Molecular Clouds, Stellar Envelopes, Cosmic Dust, Hydrocarbons, Hydrocyanic Acid

Scientific paper

The expected abundance of the most important molecules is calculated as
a function of the distance from an early-type star embedded in a dense
cloud. The C2H and HCN molecules could serve as indicators of young B
stars concealed from the observer by a thick dust layer.

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