dc.contributor.author |
Meru, Farzana |
de_DE |
dc.date.accessioned |
2013-07-17T12:50:31Z |
|
dc.date.available |
2013-07-17T12:50:31Z |
|
dc.date.issued |
2013 |
de_DE |
dc.identifier.issn |
0004-637X |
de_DE |
dc.identifier.uri |
http://hdl.handle.net/10900/36010 |
|
dc.language.iso |
en |
en |
dc.publisher |
Iop Publishing Ltd |
de_DE |
dc.relation.uri |
http://dx.doi.org/10.1088/0004-637X/764/2/146 |
de_DE |
dc.rights |
info:eu-repo/semantics/closedAccess |
|
dc.subject.ddc |
520 |
de_DE |
dc.subject.ddc |
530 |
de_DE |
dc.title |
From dust to planetesimals : an improved model for collisional growth in protoplanetary disks |
de_DE |
dc.type |
Article |
de_DE |
utue.quellen.id |
20130315161744_00040 |
de_DE |
utue.personen.roh |
Garaud, Pascale |
de_DE |
utue.personen.roh |
Meru, Farzana |
de_DE |
utue.personen.roh |
Galvagni, Marina |
de_DE |
utue.personen.roh |
Olczak, Christoph |
de_DE |
dcterms.isPartOf.ZSTitelID |
Astrophysical Journal |
de_DE |
dcterms.isPartOf.ZS-Issue |
Article 146 |
de_DE |
dcterms.isPartOf.ZS-Volume |
764 |
de_DE |
utue.fakultaet |
07 Mathematisch-Naturwissenschaftliche Fakultät |
de_DE |