From dust to planetesimals
An improved model for collisional growth in protoplanetary disks
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Date
2013-02Type
- Journal Article
ETH Bibliography
yes
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Publication status
publishedExternal links
Journal / series
The Astrophysical JournalVolume
Pages / Article No.
Publisher
IOP PublishingSubject
Accretion, accretion disks; Methods: numerical; Planetary systems; Planets and satellites: formation; Protoplanetary disksOrganisational unit
03829 - Meyer, Michael R. (ehemalig)
Notes
Received 31 August 2012, accepted for publication 13 Dezember 2012, Published 1 Februar 2013.More
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ETH Bibliography
yes
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