Table 5: Core properties determined from greybody fits to the SCUBA and IRAS HIRES sub-mm and far-infrared fluxes.
Source ID $T_{\rm d}$ M $\log(n)$ A_V A_K

(K) $M_\odot$ cm^-3

SFO 11 SMM1 23 20.6 4.6 11.5 1.3

SFO 11 SMM2 32 4.9 4.4 5.4 0.6

SFO 11 SMM3 27 3.1 4.2 3.5 0.4

SFO 11NE SMM1 23 13.4 4.6 10.2 1.1

SFO 11NE SMM2 11 26 5.4 45.7 5.1

SFO 11E SMM1 23 18.7 4.6 11.2 1.3

SFO 11E SMM2 76 1.1 4.4 3.4 0.4

SFO 11E SMM3 19 7.7 5.3 25.8 2.9

**Table 5:** Core properties determined from greybody fits to the SCUBA and IRAS HIRES sub-mm and far-infrared fluxes.
Source ID	$T_{\rm d}$	M	$\log(n)$	A_V	A_K
	(K)	$M_\odot$	cm^-3
SFO 11 SMM1	23	20.6	4.6	11.5	1.3
SFO 11 SMM2	32	4.9	4.4	5.4	0.6
SFO 11 SMM3	27	3.1	4.2	3.5	0.4
SFO 11NE SMM1	23	13.4	4.6	10.2	1.1
SFO 11NE SMM2	11	26	5.4	45.7	5.1
SFO 11E SMM1	23	18.7	4.6	11.2	1.3
SFO 11E SMM2	76	1.1	4.4	3.4	0.4
SFO 11E SMM3	19	7.7	5.3	25.8	2.9

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