The following document lists the file abstract/RHURT_1378.abs
from catalogue VI/111.
A plain copy of the file
(without headers/trailers) may be downloaded.
We propose to make fully-sampled maps of the Serpens Cloud Core at three different wavelengths using the PHT-C arrays. Our goal is to obtain high-resolution images of the protostellar sources in this cluster, including the Class 0 sources which represent the earliest observable stage of star formation. By resolving the individual sources we can obtain flux densities at 60, 100, and 160 um. Combined with existing mm & submm photometry, the ISO results will allow us to accurately determine the spectral energy distribution of these protostars and determine their temperatures, luminosities, and dust masses. ISO imaging is necessary to properly identify and separate the closely spaced ( 1') Class I and candidate Class 0 sources in this actively star- forming cloud core.