MIDINFRARED IMAGING SPECTROSCOPY IN OPHIUCHUS

The dust emission spectrum between 5 and 16 mu m has been measured at the northern edge of the dense cloud in Ophiuchus at a position where the radiation field intensity is estimated to be 10-20 times the mean Solar neighborhood value. The spectrum shows the well known emission b ands at 6.2, 7.7, 8.6, 11.3 and 12.7 mu m. ISO allows to detect the em ission features for a radiation field intensity two orders of magnitud e smaller than in the objects previously observed. Since all of these bands are considered to be characteristic of C-C or C-H bonds in aroma tic hydrocarbons this observation strongly supports the existence of l arge aromatic molecules in the general interstellar medium. An importa nt result of the observation is the presence of a significant continuu m below the features at all wavelengths, and in particular, a featurel ess continuum between the 8.6 and 11.3 mu m features and beyond that a t 12.7 mu m. The Ophiuchus spectrum is remarkably similar to that meas ured in NGC 7023. We argue that both the bands and the continuum emiss ion must come from molecules or small aggregates with less than a few hundred carbon atoms.