Laboratory detection of HC9N using a Fourier transform microwave spectrometer

Astronomy and Astrophysics – Astronomy

Scientific paper

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Cyano Compounds, Interstellar Gas, Microwave Spectra, Radio Sources (Astronomy), Absorption Spectra, Fabry-Perot Spectrometers, Fourier Transformation, Line Spectra, Microwave Radiometers

Scientific paper

The laboratory microwave spectrum of a linear carbon chain molecule, HC9N (cyano-octatetra-yne), has been observed for the first time by discharging a mixture of vinyl-cyanide and acetylene diluted in argon. The absorption spectrum was observed in a supersonic beam, using a pulsed-nozzle Fabry-Perot-type Fourier transform microwave spectrometer. Frequencies of 11 rotational transitions have been combined with the previously reported astronomical data, yielding accurate ground state parameters, B0 = 290.518322(57) MHz and D0 = 0.874(78) Hz.

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