The following document lists the file abstract/FVIALLEF_M33_CVF.abs
from catalogue VI/111.
A plain copy of the file
(without headers/trailers) may be downloaded.
NGC 604 is the brightest star-formation complex in the nearby spiral M 33. It will be observed in the central programme with CAM (filter imaging), PHOT, LWS and SWS. In order to help interpret the CAM filter imaging and obtain more information on the properties of gas and dust in this complex object, we propose an observation with the CAM CVF: it will map unambiguously the different Unidentified Infrared Bands and several fine-structure lines, which are not well separated by the CAM filters. We expect to see a wealth of details with the resolution of 6".