The A(2)Piu-X(2)Pig electrdnic system of gaseous C-7(-) is examined experim
entally in the light-of theoretical predictions. Ab initio calculations at
the RHF, RCCSD(T) and MRCI levels using the aug-cc-pVQZ basis set indicate
that the transition is accompanied by a small elongation in the molecule an
d a significant reduction in the spin-orbit coupling constant. On the basis
of these predictions the band profiles of the 0(0)(0), 1(0)(1), 2(0)(1) an
d (1)(0) transitions were recorded using photodetachment spectroscopy. Thes
e spectra revealed the spin-orbit component bands for each transition as we
ll as providing band contourswhich show partially resolved rotational struc
ture. The experimental spectra are compared to simulations based upon the c
alculated spectroscopic constants and the possible causes of the main featu
res in the band contours are accessed by least-squares fitting of the profi
les for the 0(0)(0) and 1(0)(1) transitions. The implications for the recen
t observation of coincidences between the A(2)Pi (u)-X(2)Pig vibronic bands
of C-7(-) and the diffuse interstellar bands are discussed. (C) 2000 Ameri
can Institute of Physics. [S0021-9606(00)01945-0].