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Dust Coagulation in Infalling Protostellar Envelopes I. Compact Grains

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dc.contributor.author Yorke, H. en_US
dc.contributor.author Suttner, G. en_US
dc.contributor.author Lin, D. en_US
dc.date.accessioned 2004-09-24T16:17:32Z
dc.date.available 2004-09-24T16:17:32Z
dc.date.issued 1999-07 en_US
dc.identifier.citation Astrophysical Journal en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 99-1153 en_US
dc.identifier.uri http://hdl.handle.net/2014/17716
dc.description.abstract Dust plays a key role in the optical, thermodynamic and gas dynamical behavior of collapsing molecular cores. Because of relative velocities of the individual dust grains, coagulation and shattering can modify the grain size distribution and due to corresponding changes in the medium's opacity significantly influence the evolution during early phase of star formation. en_US
dc.format.extent 912209 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other hydrodynamics radiation transfer circumstellar matter star formation dust properties en_US
dc.title Dust Coagulation in Infalling Protostellar Envelopes I. Compact Grains en_US


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