Modeling the structure, chemistry and appearance o

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Modeling the structure, chemistry and appearance of protoplanetary disks Ringberg April 13 - April 17, 2004 Carsten Dominik Disk dissipation Coincidence NIR/submm disappearance of disks (Cathie Clarke). Both measure dust. Inner disk emptied by accretion Outer disk by photo evaporation Connection because photo evaporation at rg stops feeding the inner disk. Questions Does flushing the gas necessarily flush the dust in the outer regions? Jupiter formation may require gas out to >10Myrs (David Hollenbach) Can this gas be detected (David Hollenbach, Inga Kamp, Hideko Nomura) External photoevaporation (Sabine Richling)


Type: ppt

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