The following document lists the file abstract/MFHAAS_VCD_N205.abs
from catalogue VI/111.
A plain copy of the file
(without headers/trailers) may be downloaded.
Previous scans with PHT C200 revealed that the elliptical dwarf galaxy N205 is spatially resolved in the FIR and that the SED rises steeply between 150 and 205micron indicating a large amount of very cold dust about 8-10K (Fig.1). This result, however, relies essentially on the 205micron data and may be influenced by the uncertain background determination. The scans did not cover sufficient background around N205, because they were designed for M31 (Fig.2). Therefore we need more observations to verify this unique very cold dust discovery with ISO.