The detection of interstellar vinyl cyanide /acrylonitrile/

Details The detection of interstellar vinyl cyanide /acrylonitrile/ The detection of interstellar vinyl cyanide /acrylonitrile/

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...195l.127g&link_type=abstract

Astrophysical Journal, vol. 195, Feb. 1, 1975, pt. 2, p. L127-L130.

Astronomy and Astrophysics

Astronomy

30

Acrylonitriles, Interstellar Radiation, Masers, Microwave Spectra, Molecular Spectra, Electron Transitions, Emission Spectra, Line Spectra, Radio Astronomy

Scientific paper

Interstellar vinyl cyanide, H2C CH-CN, has been discovered in its
2(11)-2(12) (1372 MHz) transition in Sgr B2. The line is in emission
with a peak antenna temperature of 0.036 K. It probably results from
maser amplification of the continuum. The total molecular content is
uncertain.

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