  We study Galactic emission foreground contamination of the OVRO and UCSB
South Pole 1994 cosmic microwave background (CMB) anisotropy data by
cross-correlating with templates of infrared dust emission and new high
resolution $H_{\alpha}$ data. $H_{\alpha}$ data provide rough upper limits on
the level of free-free emission in the data sets. The cross-correlation
analysis does not contradict a two component foreground emission hypothesis,
with the two dust-correlated components being free-free emission and spinning
dust emission.
