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Table 1:

Description of the observed fields.

IRASa
RA(2000) Dec(2000) Total gas massb Total mass in dense gasc Cluster stellar massd
source     ($M_{\odot}$) ($M_{\odot}$) ($M_{\odot}$)
IRAS08438-4340 (IRS16) 08:45:35.8 -43:51:00 99 105 103
IRAS08448-4343 (IRS17) 08:46:35.0 -43:54:30 48 88 90
IRAS08470-4243 (IRS18) 08:48:47.7 -42:54:22 (e) (f) 89
IRAS08476-4306 (IRS20) 08:49:26.6 -43:17:13 13 21 70
IRAS08477-4359 (IRS21) 08:49:32.9 -44:10:47 219 60 68
IRAS08485-4419 (IRS22) 08:50:20.7 -44:30:41 (e) (f) >38g

Notes. (a) Also listed the nomenclature used by Liseau et al. (1992); (b) derived from CO(1-0) and 13CO(2-1) observations by Elia et al. (2007); (c) derived from continuum 1.2 mm observations by Massi et al. (2007); (d) estimated by Massi et al. (2006); (e) found CO(1-0) emission (Liseau et al. 1992); (f) found a dense core at 1.2 mm centred at the cluster (Massi, private comm.); (g) inferred from the data in Massi et al. (2003).


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