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Low-mass stars
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Stellar evolution models for Z = 0.0001 to 0.03
We have calculated a grid of empirically well tested evolutionary tracks with masses M between 0.5 and 50M_{sun}_, spaced by approximately 0.1 in log M, and with metallicities... -
Variations on debris disks. II.
We describe comprehensive calculations of the formation of icy planets and debris disks at 30-150AU around 1-3M_{sun}_ stars. Disks composed of large, strong planetesimals... -
Predicted IR excesses for protoplanetary disks
We describe calculations for the formation of icy planets and debris disks at 30-150AU around 1-3M_{sun} stars. Debris disk formation coincides with the formation of planetary...
