Infrared Space Observatory (ISO) Long Wavelength Spectrometer (LWS) an
d ground-based Fabry-Perot imaging spectroscopic observations are used
to penetrate the extinction to the powerful burst of star formation t
hat has occurred in the extranuclear molecular cloud complex in the ga
laxy overlap region of the galaxies NGC 4038/39 (''The Antennae''). Pa
rameters of the starburst and typical molecular cloud core characteris
tics are derived. It is found that the starburst can power the infrare
d luminosity of this galaxy system.