dc.contributor.author |
Suttner, G. |
en_US |
dc.contributor.author |
York, H. W. |
en_US |
dc.date.accessioned |
2004-09-23T18:16:23Z |
|
dc.date.available |
2004-09-23T18:16:23Z |
|
dc.date.issued |
2001-04-18 |
en_US |
dc.identifier.citation |
Astrophysical journal, vol. 551, no. 1, pp.461-477 |
en_US |
dc.identifier.citation |
Pasadena, CA USA |
en_US |
dc.identifier.clearanceno |
00-0811 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2014/14383 |
|
dc.description.abstract |
We investigate dust dynamics and evolution during the formation of a protostellar accretion disk around intermediate-mass stars via two-dimensional numerical simulations. |
en_US |
dc.format.extent |
619207 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en_US |
|
dc.subject.other |
Solar nubula hydrodynamicscoagulation clouds |
en_US |
dc.title |
Early dust evolution in protosellar accretion disks |
en_US |