  We compute the cosmic microwave background (CMB) anisotropy in a low-density,
flat, cosmological constant, cold dark matter model which is normalized to the
two-year COBE DMR sky map. Although conclusions regarding model viability must
remain tentative until systematic effects are better understood, there are mild
indications that these models have more intermediate scale power than is
indicated by presently available CMB anisotropy observational data, with old
($t_0 \geq 15-16$Gyr), high baryon density ($\Omega_B \geq 0.0175 h^{-2}$), low
density ($\Omega_0 \sim 0.2-0.4$) models doing the worst.
