- Table 3:
parameters of the submm detections resolved by this survey. The mass of
each clump is calculated from the 850 m integrated flux value,
assuming the dust grains have thin ice mantles, and using a 100:1
gas-to-dust ratio. The column density refers to the total gas column
density (i.e. n(H+H2)).
- Table 4:
Parameters used for a three Gaussian component description of the JCMT
- Table 5:
Stellar IMF, taken from Kroupa (2001). The
third and fourth columns tabulate the contribution of each object type
to the population and mass total.
- Table 1:
Positions of the IRAS point sources satisifying the Sridharan et al. (2002) criteria, precessed to J2000 co-ordinates, alongside the kinematic distance of the IRAS source and date(s) of observation. All sources were observed during the spring and summer of 2000. All distances are taken from Sridharan et al. 2002 with the exception of IRAS 18449-0158, for which we derive the kinematic distance using
from the CS(2-1) observations of Bronfman et al. (1996). Candidates with only the far kinematic distance listed have had their distance uncertainty resolved.