The cyanomethylidyne radical has been the subject of a wide variety of studies of its spectra and reactivity
relevant to astrochemistry.
Volosatova et al. explored the
possible formation of CCN from irradiation of acetonitrile (methyl cyanide).
Reactions of CCN with various atoms and molecules have been characterized: with H
(Loison & Hickson), with N
(Stubbing et al), with H2S
(Dong et al.), with H2S, PH3, and HCl
(Wang et al.), with methane
(Wang et al.), with various alcohols
(Zhu et al.), and with various alkanes
(Zhu et al.).
The rovibrational spectrum of CCN was predicted by
Hill et al., while its Renner-Teller
splitting was studied by both
Muzangwa & Reid and
Coudert et al..
Chefai et al. chacterized the
collisional excitation of CCN by He
as well as the impact of He on its
fine and hyperfine excitation.
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While the bonding in the CCN radical can be viewed as consisting of a single bond between the two
C atoms and a
triple bond between the C and N atoms, the electrons can also
be coupled to give two double bonds as shown in the
orbital coupling diagrams
in the figure to the right. The existence of a second
resonance configuration means
that there is unpaired electron character on both of the terminal atoms, as depicted in the orbital
shown here. While much of the unpaired electron character is on the terminal C atom, the N atom also
has unpaired electron character. Both terminal atoms can form covalent bonds, yield HCCN and CCNH.
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