Mid-Infrared Imaging Spectroscopy in Ophiuchus
F. Boulanger, W. T. Reach, A. Abergel, J. P. Bernard, C. J. Cesarsky, D. Cesarsky, F. X. Desert, E. Falgarone, J. Lequeux, L. Metcalfe, M. Perault, J. L. Puget, D. Rouan, M. Sauvage, D. Tran, L. Vigroux;
AaA, 1996, 315, L325
ABSTRACT: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 bands at 6.2, 7.7,
8.6, 11.3 and 12.7{mu}m.
ISO allows to detect the emission features for a
radiation field intensity two orders of magnitude 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 aromatic hydrocarbons this observation strongly
supports the existence of large aromatic molecules in the general interstellar
medium.
An important result of the observation is the presence of a significant
continuum below the features at all wavelengths, and in particular, a
featureless continuum between the 8.6 and 11.3{mu}m features and beyond that at
12.7{mu}m.
The Ophiuchus spectrum is remarkably similar to that measured in NGC
7023.
We argue that both the bands and the continuum emission must come from
molecules or small aggregates with less than a few hundred carbon atoms.
KEYWORDS: infrared: general, ism: lines and bands, continuum, ism: general, dust, extinction, individual: {rho} oph
PERSOKEY:mir, dust, pah, iso, h2, ,
CODE: boulanger96a