Characterising discs around Herbig Ae/Be stars through modelling of low-J 12CO lines

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Table 1:

Stellar properties^a and the derived dust mass of the discs.
#	Source	Distance	Spectral type	Luminosity	$M_{\rm star}$	$F_{\rm 1.3~mm}^{c}$	$T_{\rm avg}$	$M_{\rm {dust}}$
		(pc)		( $L_{\odot}$ )	( $M_{\odot}$ )	(mJy)	(K)	( $10^{-4}~M_{\odot}$ )
(1)	HD 100546	103	B9	36	2.5	470	30-40	2.1-2.9
(2)	HD 179218	240	B9	80	2.7	71	30-40	1.7-2.4
(3)	V892 Tau^b	-	B8 V	400	5.5	230	-	-
(4)	AB Aur	144	A0	47	2.5	100	30-40	0.9-1.2
(5)	HD 163296	122	A1-A3	30	2.4	780	30-40	4.9-6.9
(6)	HD 169142	145	A5	32	2.5	169^d	30-40	1.5-2.1
(7)	HD 139614	157	A7	12	1.8	240	30-40	2.5-3.5
(8)	HD 142666	116	A7-A8	11	1.8	127	30-40	0.7-1.0
(9)	HD 135344	84	F4-F8	3	1.3	140	30-40	0.4-0.6

^a See Table 3 of Dominik et al. (2003), and references therein. ^b Binary system with two B8 V stars with total mass of 5.5 $M_{\odot}$ (Smith et al. 2005; Palla & Stahler 1993; Monnier et al. 2008). ^c Mannings & Sargent (1997), unless noted otherwise. ^d Raman et al. (2006).

Source LaTeX | All tables | In the text

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