  We present 0".97 $\times$ 0".53 (470 pc $\times$ 250 pc) resolution CO ($J$ =
2-1) observations toward the nearby luminous merging galaxy NGC 6240 with the
Atacama Large Millimeter/submillimeter Array. We confirmed a strong CO
concentration within the central 700 pc, which peaks between the double nuclei,
surrounded by extended CO features along the optical dust lanes ($\sim$11 kpc).
We found that the CO emission around the central a few kpc has extremely broad
velocity wings with full width at zero intensity $\sim$ 2000 km s$^{-1}$,
suggesting a possible signature of molecular outflow(s). In order to extract
and visualize the high-velocity components in NGC 6240, we performed a multiple
Gaussian fit to the CO datacube. The distribution of the broad CO components
show four extremely large linewidth regions ($\sim$1000 km s$^{-1}$) located
1-2 kpc away from both nuclei. Spatial coincidence of the large linewidth
regions with H$\alpha$, near-IR H$_2$, and X-ray suggests that the broad CO
(2-1) components are associated with nuclear outflows launched from the double
nuclei.
