Cyanoallene, CH2=C=CH-CN - Astrophysical predictions

Details Cyanoallene, CH2=C=CH-CN - Astrophysical predictions Cyanoallene, CH2=C=CH-CN - Astrophysical predictions

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...161..327s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 161, no. 2, June 1986, p. 327, 328.

Astronomy and Astrophysics

Astronomy

Cyano Compounds, Interstellar Matter, Molecular Clouds, Radio Astronomy, Astronomical Spectroscopy, Isomers, Millimeter Waves

Scientific paper

Based on microwave and recent laboratory measurements in the millimeter wave region between 85 and 180 GHz, higly precise frequency predictions for an isomer of methylcyanoacetylene, cyanoallene (CH2=C=CH-CN) are reported, with application to the prediction of formation mechanisms. The selected transitions with low k can be excited in warm interstellar clouds, and could be detected if the column density were sufficiently high. A possible interstellar formation mechanism of the various C4H4N(+) isomers is suggested.

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