HCN emission from OH infrared sources

Details HCN emission from OH infrared sources HCN emission from OH infrared sources

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985natur.317..336d&link_type=abstract

Nature (ISSN 0028-0836), vol. 317, Sept. 26, 1985, p. 336-338.

Computer Science

30

Hydrocyanic Acid, Hydroxyl Emission, Infrared Stars, Late Stars, Radio Emission, Carbon Monoxide, Stellar Envelopes

Scientific paper

Radio emission of the HCN molecule has been considered to be a tracer of carbon-rich circumstellar environments. The authors report, however, the detection of HCN radio emission from oxygen-rich late type stars. These results relate to the issue of the progenitors for planetary nebulae. The presence of the HCN molecule in oxygen-rich stars suggests that complex photochemical reactions are proceeding in the outer circumstellar envelope of late type stars.

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