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Home All issues Volume 497 / No 1 (April I 2009) A&A, 497 1 (2009) 117-136 Full HTML
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This article has an erratum: [https://doi.org/10.1051/0004-6361/200810401e]

 

 

Table A.13:

Compilation of disks masses1.
Name Spectral Luminosity Teff Distance Star mass Age $\lambda$ Flux Disk mass
  type ($L_\odot$) (K) (pc) ($M_\odot$) (Myr) (mm) (mJy) ($M_\odot$)
AB Aur A0 49 9500 144 2.57 3.87 1.4 85 0.0278
HD 100546 B9 45 10 500 103 2.53 5.59 1.3 465 0.0540
HD 142527 F6 69 6300 200 3.54 1.11 1.3 1190 1.4860
HD 179218 / MWC 614 B9 500 10 000 240 5.02 0.473 1.3 71 0.0447
HD 100453 A9 8 7400 114 1.66 14.1 1.2 270 0.0709
CD-36 10010B F8 8 6200 84 1.63 9.49 1.3 142 0.0345
HD 139614 A7 11 7800 157 1.83 10.7 1.3 242 0.1293
HD 169142 B9 44 10 500 145 2.5 5.69 1.3 169 0.0389
HD 142666 A8 8 7500 116 1.65 14.9 1.2 79 0.0201
HD 144432 A9 32 7300 200 2.26 3.87 1.3 37 0.0369
HD 150193 / MWC 863 A1 30 9500 150 2.25 6.10 1.3 45 0.0143
HD 163296 A1 36 9500 122 2.49 5.79 1.3 705 0.1485
HD 34282 A0 36 9500 400 2.49 5.79 1.3 110 0.2259
HD 35187 A2 34 9100 150 2.43 4.65 1.2 20 0.0055
UX Ori A3 42 8600 430 2.43 4.22 1.2 19.8 0.0481
CQ Tau F2 5 6800 100 1.49 769 1.3 143 0.0415
MWC 758 A3 21 8500 200 2.17 6.26 1.3 72 0.0471
LkH$\alpha $259 A9 107 7320 850 3.6 1.17 2.6 <6 <0.722
WW Vul A3 43 8600 550 2.44 4.19 1.2 9.1 0.0362
BF Ori A5 34 8300 450 2.34 4.37 1.3 6 0.0228
SV Cep A0 14 8600 715 1.91 11.7 1.3 7 0.0459
V376 Cas B5 190 13 800 600 3.77 2.66 2.7 <5 <0.089
LkH$\alpha $198 B7 210 12 000 600 3.51 1.49 2.7 <5 <0.1141
VY Mon B8 1400 10 700 800 6.9 0.243 1.3 120 0.6874
HD 97048 A0 44 10 000 150 2.53 4.61 1.3 452 0.1305
LkH$\alpha $234 B5 800 14 500 1250 5.01 0.524 1.3 <20 <0.181
T Ori A3 83 8500 460 2.92 2.49 1.3 <6 <0.021
V380 Ori B9 100 9500 460 3.05 2.00 1.3 <24 <0.056
LkH$\alpha $218 B9 107 10 700 1150 2.97 2.77 1.3 <27 <0.3906
Elias 3-1 A6 21 8000 140 2.06 6.11 2.7 45 0.1360
BD+404124 B2 5900 22 000 1000 - - 2.7 <5 <0.133
V1686 Cyg B5 1820 15 500 1000 6.05 0.312 2.7 <5 <0.246
BD+61154 B8 225 11 800 650 3.88 1.43 2.7 11.2 0.3509
RR Tau A4 150 8800 800 3.57 1.34 1.3 <20 <0.224
HD 200775 B2 1900 18 500 600 6.9 0.337 1.3 <6 <0.007
MWC 480 A3 25 8500 130 2.19 5.98 1.4 235 0.0797
HD 34700 G0 20 6000 90 2.36 3.39 1.35 11.7 0.0037
MWC 297 B1.5 10 700 24 000 250 9 1 1.3 168.6 0.0323
Z CMa B8 9200 20 000 930 12 0.05 1.4 24.1 0.2307
R Mon B0 5600 25 000 800 8 1 1.4 8.3 0.0093
MWC 1080 B0 5600 25 000 1000 10 1 1.4 2.1 0.0036
MWC 137 B0 15 000 26 000 1300 14 1 1.4 7.1 <0.007
VV Ser A0 50 10 000 260 2.68 3.87 1.3 1.44 0.0012
LkH$\alpha $ 215 B7.5 5300 22 000 800 7 0.4 1.4 <1.5 <0.009
1 The flux shown is the excess at 1.3 mm subtracting the free-free contribution in our sources. In MWC 297 we have used the flux of Manoj et al. (2007). References for the mm fluxes are: Acke et al. (2004), Alonso-Albi et al. (2008), di Francesco et al. (1997), Fuente et al. (2003), Fuente et al. (2006), Henning et al. (1994), Henning et al. (1998), Mannings et al. (1997), Mannings et al. (2000), Natta et al. (1997), Natta et al. (2001), Piétu et al. (2003), Piétu et al. (2006), Sylvester et al. (2001).

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