Radiative Transfer in Protoplanetary Disks
Radiative Transfer in Protoplanetary Disks
Radiative Transfer in Protoplanetary Disks
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≈ 400 000 models<br />
Some parameters<br />
fixed from data<br />
(amax, Mdust, Rout)<br />
→Fitt<strong>in</strong>g for 6<br />
parameters<br />
IM Lupi: quantitative constra<strong>in</strong>ts<br />
Bayesian method to estimate model parameters:<br />
for SED + mm visibilities<br />
P<strong>in</strong>te et al 2008<br />
Probability<br />
Probability Probability Probability Probability Probability<br />
1.0<br />
0.5<br />
0.0<br />
1.0<br />
0.6<br />
0.4<br />
0.2<br />
0.5<br />
cos(i)<br />
0.0<br />
0.05 0.1 0.2 0.5 1.0<br />
r<strong>in</strong><br />
1.0<br />
0.5<br />
0.0<br />
0.0<br />
1.0<br />
0.5<br />
0.0<br />
0<br />
−1<br />
−2<br />
5 10 15<br />
1.0<br />
0.5<br />
0.0<br />
0.6<br />
0.4<br />
0.2<br />
1.0 1.1 1.2<br />
surface density flar<strong>in</strong>g<br />
0.0<br />
0.00 0.05 0.10 0.15 0.20<br />
H stratification<br />
See also Glauser et al 2008, Bouy et al 2008, Duchêne et al 2010
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