We have mapped several nearby galaxies in the CO(4-3) line transition with
the Heinrich-Hertz-Telescope on Mt. Graham, Arizona, during an excellent we
ather period in December 1998. Here we report on our observations of M51 an
d NGC 6946. The results suggest a concentration of highly excited CO gas to
the nuclei of these galaxies. Moreover, in both objects CO(4-3) line emiss
ion was also detected for the first time in the spiral arms, several kilopa
rsecs away from the centre.