Photofragmentation of mass-selected C-16(+) to C-36(+) clusters is inv
estigated at two laser wavelengths: 532 and 355 nm. The depletion depe
ndence on laser fluence leads to the number of absorbed photons, toget
her with the photoabsorption cross section. From the knowledge of the
internal energy deposited in the clusters before the fragmentation ste
p, the dissociation energies are deduced. Clusters C-16(+) to C-29(+)
are found to be less and less stable, whereas above C-30(+) an increas
ed stability is observed.