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The outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals? III. Sedimentation driven coagulation inside the snow-line
Methods Numerical Planets satellites formation Protoplanetary disks
2011/10/20
We investigate dust growth due to settling in a 1D vertical column of a protoplanetary disk. It is known from the observed 10 micron feature in disk SEDs, that small micron-sized grains are present at...
The Optical-NIR Opacity Law in YSO Disks and Envelopes：Evidence for Dust Growth?
YSO Disks Dust Growth
2009/6/18
The Optical-NIR Opacity Law in YSO Disks and Envelopes：Evidence for Dust Growth?
The Optical-NIR Opacity Law in YSO Disks and Envelopes：Evidence for Dust Growth?
YSO Disks Dust Growth
2009/6/16
The Optical-NIR Opacity Law in YSO Disks and Envelopes：Evidence for Dust Growth?