The singlet and triplet states of AlCu and AlAg below about 32 000 cm(
-1) are studied using the internally contracted multireference configu
ration-interaction method. A more elaborate study of the X (1) Sigma() ground state of AlCu is undertaken using extended Gaussian basis set
s, including the effect of inner-shell correlation and including a per
turbational estimate of relativistic effects. Our best estimate of the
spectroscopic constants (r(0), Delta G(1/2), and D-0) for the X (1) S
igma(+) state with the experimental values in parentheses are: 4.416(4
.420) a0, 295(294) cm(-1), and 2.318(2.315) eV. The calculations defin
itively assign the upper state in the observed transition at 14 892 cm
(-1) to the lowest (1) Pi. state. The calculated spectroscopic constan
ts and radiative lifetime for the (1) Pi state are in good agreement w
ith experiment. The calculations support the tentative assignments of
Behm et al. for three band systems observed in the visible region betw
een 25 000 and 28 000 cm(-1). However, the computed spectroscopic cons
tants are in very poor agreement with those deduced from an analysis o
f the spectra. Analogous theoretical results for AlAg suggest that the
(2)(3) Pi, (3)(3) Pi, and (3)(1) Sigma(+) states account for the band
s observed, but not assigned, by Duncan and co-workers.