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dc.contributor.author
Garaud, Pascale
dc.contributor.author
Meru, Farzana
dc.contributor.author
Galvagni, Marina
dc.contributor.author
Olczak, Christoph
dc.date.accessioned
2017-06-10T11:51:29Z
dc.date.available
2017-06-10T11:51:29Z
dc.date.issued
2013-02
dc.identifier.issn
0004-637X
dc.identifier.other
10.1088/0004-637X/764/2/146
dc.identifier.uri
http://hdl.handle.net/20.500.11850/59857
dc.language.iso
en
dc.publisher
IOP Publishing
dc.subject
Accretion, accretion disks
dc.subject
Methods: numerical
dc.subject
Planetary systems
dc.subject
Planets and satellites: formation
dc.subject
Protoplanetary disks
dc.title
From dust to planetesimals
dc.type
Journal Article
ethz.title.subtitle
An improved model for collisional growth in protoplanetary disks
ethz.journal.title
The Astrophysical Journal
ethz.journal.volume
764
ethz.journal.issue
2
ethz.journal.abbreviated
Astrophys. J.
ethz.pages.start
146
ethz.size
19 p.
ethz.notes
Received 31 August 2012, accepted for publication 13 Dezember 2012, Published 1 Februar 2013.
ethz.identifier.nebis
000001169
ethz.publication.place
Bristol
ethz.publication.status
published
ethz.leitzahl
ETH Zürich::00002 - ETH Zürich, direkt::00012 - Lehre und Forschung, direkt::00007 - Departemente, direkt::02010 - Departement Physik / Department of Physics::02504 - Institut für Astronomie / Institute of Astronomy::03829 - Meyer, Michael R. (ehemalig)
ethz.leitzahl.certified
ETH Zürich::00002 - ETH Zürich, direkt::00012 - Lehre und Forschung, direkt::00007 - Departemente, direkt::02010 - Departement Physik / Department of Physics::02504 - Institut für Astronomie / Institute of Astronomy::03829 - Meyer, Michael R. (ehemalig)
ethz.date.deposited
2017-06-10T11:51:40Z
ethz.source
ECIT
ethz.identifier.importid
imp59365017875cb55756
ethz.ecitpid
pub:95695
ethz.eth
yes
ethz.availability
Metadata only
ethz.rosetta.installDate
2017-07-12T22:59:20Z
ethz.rosetta.lastUpdated
2019-02-02T06:06:23Z
ethz.rosetta.exportRequired
true
ethz.rosetta.versionExported
true
ethz.COinS
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