The following document lists the file abstract/RLISEAU_SERPSPEC.abs
from catalogue VI/111.
A plain copy of the file
(without headers/trailers) may be downloaded.
Mapping with the LWS of the two central dense cores of the Serpens molecular cloud is proposed. One of the cores is currently forming a cluster of low to intermediate mass stars at very high efficiency, whereas the other one appears relatively inactive and may be in an earlier phase of stellar formation. Full grating scans with the LWS offer the opportunity to study simultaneously the physical state of the gas and the dust and to unvey possible differences between the cores. The proposed programme is aimed at a complete and homogeneous ISO data base for a number of star forming regions. We seek to complement CAM and PHOT mapping observations in the Guaranteed and Open Time by the respective instrument teams.