dc.contributor.author | Yorke, H. W. | en_US |
dc.date.accessioned | 2004-09-23T21:11:12Z | |
dc.date.available | 2004-09-23T21:11:12Z | |
dc.date.issued | 2000-06-21 | en_US |
dc.identifier.citation | Star Formation 2000 | en_US |
dc.identifier.citation | Ringberg, Germany | en_US |
dc.identifier.clearanceno | 00-1643 | en_US |
dc.identifier.uri | http://hdl.handle.net/2014/15865 | |
dc.description.abstract | Radiative effects strongly hinder the formation of massive stars. A necessary condition for accretion growth of a hydrostatic object up to high masses is the formation of and accretion through a circumstellar disk. | en_US |
dc.format.extent | 180215 bytes | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en_US | |
dc.subject.other | star formation circumstellar disks | en_US |
dc.title | Can massive stars be formed by accretion? | en_US |