Dust properties of protoplanetary disks in the Taurus-Auriga star forming region from millimeter wavelengths

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Table 2:

Stellar properties.
Object	ST	$T_{\rm {eff}}$	$L_{\star }$	$L_{\rm {acc}}$	Ref. ( $L_{\rm {acc}}$ )	$R_\star$	${\rm Log} \ \dot{M}_{\rm {acc}}$	$M_\star$	Age
		(K)	( $L_\odot$ )	( $L_\odot$ )		( $R_{\odot}$ )	( $M_\odot$ yr^-1)	( $M_\odot$ )	(Myr)
AA Tau	K7	4060	0.80	0.03	1	1.8	-8.56	0.8	2.4
CI Tau	K7	4060	1.01	0.11	2	2.0	-7.95	0.8	1.7
CW Tau	K3	4730	1.32	0.05	2	1.7	-8.58	1.2	6.6
CX Tau	M2.5	3488	0.48	0.03	2	1.9	-8.18	0.3	0.8
CY Tau	M1	3705	0.55	0.04	1	1.8	-8.24	0.5	1.4
DE Tau	M2	3560	1.01	0.07	1	2.6	-7.69	0.4	0.2
DL Tau	K7	4060	0.89	0.23	2	1.9	-7.66	0.8	2.2
DM Tau	M1	3705	0.24	0.10	2	1.2	-7.99	0.5	3.6
DN Tau	M0	3850	0.91	0.02	1	2.2	-8.55	0.6	1.1
DO Tau	M0	3850	0.79	0.60	1	2.0	-7.10	0.6	1.3
DR Tau	K7	4060	1.09	0.72	2	2.1	-7.12	0.8	1.5
DS Tau	K2	4900	0.90	0.21	1	1.3	-8.00	1.1	17.0
FM Tau	M0	3850	0.26	0.10	2	1.2	-8.13	0.6	6.3
FZ Tau	M0	3850	1.06	0.46	3	2.3	-7.14	0.6	0.8
GM Aur	K3	4730	1.26	0.07	1	1.7	-8.44	1.2	7.2
GO Tau	M0	3850	0.27	0.01	3	1.2	-9.14	0.6	4.8
HO Tau	M0.5	3778	0.16	0.01	2	0.9	-9.13	0.5	8.7
IQ Tau	M0.5	3778	0.73	0.04	2	2.0	-8.24	0.6	1.2
RY Tau	K1	5080	6.59	1.60	4	3.3	-7.03	2.2	1.1
SU Aur	G2	5860	10.6	0.55	4	3.2	-7.52	1.7	2.2
UZ Tau E	M1	3705	2.27	0.31	2	3.7	-7.02	0.5	0.1

References. (1) Gullbring et al. (1998); (2) Valenti et al. (1993), these accretion luminosities have been multiplied by a factor of (140 pc/160 pc)² to account for the current estimate of 140 pc for the distance to the Taurus-Auriga star forming region; (3) Herczeg et al. (2009, in preparation); (4) Calvet et al. (2004).

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