Laboratory Observation of Para-H2C4N

Details Laboratory Observation of Para-H2C4N Laboratory Observation of Para-H2C4N

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001apj...552..409t&link_type=abstract

The Astrophysical Journal, Volume 552, Issue 1, pp. 409-412.

Astronomy and Astrophysics

Astronomy

Molecular Data, Molecular Processes

Scientific paper

The rotational spectrum of para-H2C4N (I(H)=0) in the Ka=1 rotational level has been observed in supersonic expansion at low temperature by Fourier transform microwave spectroscopy. The C2v structure of H2C4N has been confirmed by an analysis of both the present Ka=1 transitions and the Ka=0 transitions from the previous ortho-H2C4N (I(H)=1) study. Rest transition frequencies of para-H2C4N are now available for radio-astronomical searching.

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