Hinkle K W, Keady J J, Bernath P F
Science. 1988 Sep 9;241(4871):1319-22. doi: 10.1126/science.241.4871.1319.
Vibration-rotation lines of C(3) have been identified in the circumstellar spectrum of the obscured carbon star IRC+10216. This molecule is of interest in both the chemistry of flames, where it may be involved in the formation of soot, and in astrophysics, where it is a potential building block for carbonaceous grains. This high-resolution infrared detection of the pure carbon chain molecule C(3) allows the estimation of the equilibrium C-C bond length, 1.297 angstroms. Possible astrophysical formation and destruction mechanisms for C(3) are reviewed, including the relationship between C(3) and carbon clusters.
