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Table B.1

Stellar and disk parameters available in the literature.

Name Spectral Ṁ acc R gap,in,SED R in,SED R in,mm i log LX Disk Ref
type [10-8 M⊙ yr-1] [AU] [AU] [AU] [°] [erg/s] Type
LkHα330 G3 0.20 0.8 50 68 35 ... ... 1, 12, 22, 26
DM Tau M1 0.60 ... 3 19 35 30.30 TD 1, 10, 20, 21, 28
LkCa15 K3 0.30 4 48 50 49 <29.6 PTD 1, 15, 16, 21, 24
GM Aur K5 1.00 1 24 28 55 30.20 TD 6, 9, 10, 20, 21, 28
SZ Cha K0 0.24 ... 29 ... ... 29.90 PTD 16, 17, 21, 25
TW Hya K7 0.20 ... 4 4 4 30.32 ... 10, 14, 23, 27
CS Cha K6 0.53 ... 43 ... 45 30.56 TD 10, 16, 24, 25, 30
CHXR22E M3.5 ... ... 7 ... ... 29.41 TD 16, 19
Sz18 M3 1.5e-10 ... 8 ... ... ... TD 16, 19
Sz27 M0 1.2e-9 ... 15 ... ... 29.76a PTD 16, 19
Sz45 M0.5 7.6e-10 ... 18 ... ... ... WTD 16, 19
Sz84 M5.5 1.00 ... 55 ... ... ... ... 8
RX J1615 K5 0.04 ... 3b 30 41 30.40 ... 1, 2, 8
Oph 22 M2 ... ... 1 ... ... ... ... 8
Oph 24 M0.5 1.00 ... 3 ... ... ... ... 8
SR 21 G3 <0.1 0.45 18 36 22 30.00 ... 1, 3, 4, 5, 18, 26
ISO-Oph 196 M4 0.20 ... ... 15 28 ... ... 1, 18
DoAr 44 K3 0.90 ... 27 30 35 29.9 PTD 1, 13, 29
Ser 29 M0 30.00 ... 8 ... ... ... ... 8
Ser 34 M0 0.25 ... 25 ... ... ... ... 8
RX J1842.9 K2 0.10 ... 5 ... ... 30.34 ... 6, 7, 19
RX J1852.3 K3 0.05 ... 16 ... ... 30.41 ... 6, 7, 19

Reference. (1) Andrews et al. (2011); (2) Krautter et al. (1997); (3) Brown et al. (2009); (4) Andrews et al. (2009); (5) Grosso et al. (2000); (6) Hughes et al. (2010); (7) Neuhäuser et al. (2000); (8) Merín et al. (2010); (9) Hughes et al. (2008); (10) Güdel et al. (2010); (11) König et al. (2001); (12) Brown et al. (2008); (13) Montmerle et al. (1983); (14) Hughes et al. (2007); (15) Neuhaeuser et al. (1995); (16) Kim et al. (2009); (17) White et al. (2000); (18) Natta et al. (2006); (19) Pascucci et al. (2007); (20) Ingleby et al. (2009); (21) Espaillat et al. (2010); (22) Salyk et al. (2009); (23) Herczeg & Hillenbrand (2008); (24) Ingleby et al. (2013); (25) Espaillat et al. (2013); (26) Brown et al. (2007); (27) Calvet et al. (2002); (28) Calvet et al. (2005); (29) Kim et al. (2013); (30) Pascucci & Sterzik (2009). Rgap,in,SED is the inner radius of the gap in PTDs obtained from MIR SED fitting, whereas Rin is the inner radius of the dusty outer disk, i.e. the outer radius of the gap in PTDs and of the hole in TDs.

(a)

Highly uncertain parameter.

(b)

Value corrected for the different distance as explained in Appendix A.1.

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