Radiative Transfer in Protoplanetary Disks
Radiative Transfer in Protoplanetary Disks
Radiative Transfer in Protoplanetary Disks
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ng the <strong>in</strong>ner radius of circumstellar disks<br />
Measur<strong>in</strong>g the <strong>in</strong>ner radius of disks<br />
teristic NIR size measured by <strong>in</strong>terferometers<br />
Characteristic NIR size measured by <strong>in</strong>terferometers < 1 AU:<br />
:comparabletothelocationofterrestrialplanets<strong>in</strong><br />
comparable to the location of terrestrial planets <strong>in</strong> more<br />
volved systems<br />
odel<br />
evolved systems<br />
ple emission model :<br />
R<strong>in</strong>g model:<br />
resolved central star + narrow<br />
g<br />
simple emission model:<br />
unresolved central star + narrow<br />
ative contribution from the<br />
r<strong>in</strong>g<br />
r and the disk estimated from<br />
relative contribution from star &<br />
uxdecompositionofthe<br />
disk estimated from SED<br />
ad-band SED (Millan-Gabet<br />
01)
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