Physics
Scientific paper
Aug 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phst..130a4015d&link_type=abstract
Physica Scripta, Volume 130, Issue , pp. 014015 (2008).
Physics
3
Scientific paper
The aggregation, fragmentation and thermal processing of dust in protoplanetary disks is believed to be the first step on the long road from dust to planets. Models of this process in the literature have so far been applied mostly to the early solar system, and were mostly limited to a static 'minimum mass solar nebula' model of the protoplanetary disk. We present the initial results of a campaign to extend such a modeling to evolving protoplanetary disks, to improve the realism and detail of coagulation/fragmentation models compared to models in the literature so far and to link these models to observations.
Brauer Frithjof
Dullemond Cornelis Petrus
Henning Th
Natta Antonella
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