The effects of the ultraviolet laser irradiation of [CINO](n) weakly bound
clusters, formed in a supersonic jet, are analyzed by considering three pro
cesses: the photofragmentation of bare CINO, the Cl + CINO reaction, and NO
relaxation within the cluster. The photofragmentation of jet-cooled CINO a
t 355 nm produces NO(upsilon" 1) with a kinetic energy of 2240 cm(-1), a sp
in-orbit preference of F-1/F-2 = 1.2, and A-doublet state preferences of IT
(A")/II(A") = 2.0 and 4.0 for the F-1 and F-2 manifolds, respectively. The
NO distribution of rotational states was parametrized using a Gaussian func
tion centered at N = 34, with a fwhm of 17. On the other hand, the Cl + CIN
O reaction, studied at a collision energy of 2780 cm(-1), gives NO(upsilon"
= 1) described by a Boltzmann rotational distribution with T-rot = 950 +/-
100 K. The relative population of the NO spin-orbit states is F-1/F-2 = 2.
5, with a A-doublet state preference of n(A")/II(A') = 1.2 and E-trans(NO)
of 578 cm(-1). It is found that 57% of available energy is disposed as E-in
t(Cl-2). As a result of the irradiation of the [CINO],, clusters at 355 nm
are observed: Holt;Boltzmann, ensembles of NO(v" = 1) and NO(upsilon" = 0)
molecules described by T-rot of 310 +/- 30 and 170 +/- 25 K, respectively,
with no spin-orbit or A-doublet state preferences, overlapped with a Gaussi
an distribution already assigned to the NO photofragment. The relative cont
ribution of the NO(v" = 1) photofragment to the spectra is drastically redu
ced upon increasing the backing pressure, as it undergoes translational and
rotational relaxation within the clusters. Our high-resolution studies pro
vide evidence that suggests that the reaction takes place within the [ClNO]
(n) clusters.