The analysis of the sample of southern globules investigated by Scappini et
al. in the CO (4-3) transition has been extended using a statistical equil
ibrium-radiative transfer model and making use of the results of Bourke et
al. and Henning & Launardt for those globules. CO column densities and exci
tation temperatures have been calculated and the results compared with a ch
emical model representative of the chemistry of a spherical dark cloud. In
a number of cases the gas kinetic temperatures have been constrained.