We present the first measurements of rotational distributions for phot
oionization over extended energy ranges [0 less-than-or-equal-to E(k)
less-than-or-equal-to 200 eV for N2 (2sigma(mu)-1) and of 3 less-than-
or-equal-to E(k) less-than-or-equal-to 125 eV for CO (4sigma-1)]. The
N2 and CO results show a strikingly unusual and different energy depen
dence. Although differences are expected due to the absence of a cente
r of symmetry in CO, detailed calculations reveal that this behavior a
rises from the presence of Cooper minima in the photoelectron continuu
m (ksigma(g)) in the case of N2 and from an f-wave shape resonance for
4sigma-1 photoionization in CO.