Table 5: The bolometric corrections BC_V (from Bessell et al. 1998), the luminosity L (in $10^3~L_{\odot}$ ), the distance D (in kpc) and the dust mass ( $10^{-5}~M_{\odot}$ ) are given, together with the estimated errors.
Name BC_V L D $M_{{\rm d}}$

( $10^3~L_{\odot}$ ) (kpc) ( $10^{-5}~M_{\odot}$ )

TW Cam -0.35 $3.7\pm2.6$ $3.1\pm1.1$ $3.0\pm2.2$

RV Tau
-0.49 $3.7\pm2.6$ $2.17\pm0.72$ $4.2\pm3.0$

SU Gem
-0.03 $1.20\pm0.77$ $2.11\pm0.66$ $0.45\pm0.32$

UY CMa
-0.08 $4.5\pm3.3$ $8.4\pm3.1$ $3.3\pm3.8$

U Mon
-0.24 $3.8\pm2.7$ $0.77\pm0.28$ $1.8\pm1.3$

AC Her
-0.07 $2.4\pm1.6$ $1.13\pm0.39$ $3.0\pm2.1$

R Sct
-0.52 $9.4\pm7.1$ $0.75\pm0.29$ $0.10\pm0.10$

**Table 5:** The bolometric corrections BC_V (from Bessell et al. 1998), the luminosity L (in $10^3~L_{\odot}$ ), the distance D (in kpc) and the dust mass ( $10^{-5}~M_{\odot}$ ) are given, together with the estimated errors.
Name	BC_V	L	D	$M_{{\rm d}}$
		( $10^3~L_{\odot}$ )	(kpc)	( $10^{-5}~M_{\odot}$ )
TW Cam	-0.35	$3.7\pm2.6$	$3.1\pm1.1$	$3.0\pm2.2$
RV Tau	-0.49	$3.7\pm2.6$	$2.17\pm0.72$	$4.2\pm3.0$
SU Gem	-0.03	$1.20\pm0.77$	$2.11\pm0.66$	$0.45\pm0.32$
UY CMa	-0.08	$4.5\pm3.3$	$8.4\pm3.1$	$3.3\pm3.8$
U Mon	-0.24	$3.8\pm2.7$	$0.77\pm0.28$	$1.8\pm1.3$
AC Her	-0.07	$2.4\pm1.6$	$1.13\pm0.39$	$3.0\pm2.1$
R Sct	-0.52	$9.4\pm7.1$	$0.75\pm0.29$	$0.10\pm0.10$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction: 850 ${\mu }$ m SCUBA data
	3 Spectral Energy Distributions (SEDs)
	4 An optically thin dust fit
	5 Discussion: Characteristics of the dust excess
	6 Conclusions
	References
	Online Material
	Appendix A: Photometric data