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Theory of formation of massive stars via accretion

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dc.contributor.author Yorke, Harold W.
dc.date.accessioned 2006-02-13T23:46:08Z
dc.date.available 2006-02-13T23:46:08Z
dc.date.issued 2003-07
dc.identifier.citation Star Formation at High Angular Resolution, Sydney, Australia, July 22-25, 2003 en
dc.identifier.clearanceno 03-3409
dc.identifier.uri http://hdl.handle.net/2014/38609
dc.description.abstract The collapse of massive molecular clumps can produce high mass stars, but the evolution is not simply a scaled-up version of low mass star formation. en
dc.description.sponsorship NASA en
dc.format.extent 3690253 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US en
dc.publisher Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2003. en
dc.subject stars formation en
dc.subject stars en
dc.subject high mass en
dc.subject disks en
dc.title Theory of formation of massive stars via accretion en
dc.type Preprint en


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