Table 5: Results from the dust emission modelling.
Source $T_{\star}$ $T_{\rm d}(r_{\rm i})$ $\tau_{10}$ $\chi^{2}_{\rm red}$ N

[K] [K]

LP And 2400 1100 0.55 1.6 11

CW Leo 2000 1500 1.2 2.4 12

RW LMi 2400 1200 0.6 0.9 11

V384 Per 1800 1000 0.2 0.9 10

AFGL 3068 2400 1500 4.0 5.3 11

TX Cam 2200 800 0.4 0.5 9

GX Mon 1800 500 0.3 4.9 9

WX Psc 1800 1000 3.0 1.1 12

IK Tau 2400 1200 1.2 0.9 12

IRC-10529 1800 800 3.0 3.1 10

**Table 5:** Results from the dust emission modelling.
Source	$T_{\star}$	$T_{\rm d}(r_{\rm i})$	$\tau_{10}$	$\chi^{2}_{\rm red}$	N
	[K]	[K]
LP And	2400	1100	0.55	1.6	11
CW Leo	2000	1500	1.2	2.4	12
RW LMi	2400	1200	0.6	0.9	11
V384 Per	1800	1000	0.2	0.9	10
AFGL 3068	2400	1500	4.0	5.3	11
TX Cam	2200	800	0.4	0.5	9
GX Mon	1800	500	0.3	4.9	9
WX Psc	1800	1000	3.0	1.1	12
IK Tau	2400	1200	1.2	0.9	12
IRC-10529	1800	800	3.0	3.1	10

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