Collision velocity of dust grains in self-gravitating protoplanetary discs

We have conducted the first comprehensive numerical investigation of the relative velocity distribution of dust particles in self-gravitating protoplanetary discs with a view to assessing the viability of planetesimal formation via direct collapse in such environments. The viability depends cruciall...

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Detalles Bibliográficos
Autores principales: Booth, Richard A., Clarke, Cathie J.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Oxford University Press 2016
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4914785/
https://www.ncbi.nlm.nih.gov/pubmed/27346980
http://dx.doi.org/10.1093/mnras/stw488

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4914785/
https://www.ncbi.nlm.nih.gov/pubmed/27346980
http://dx.doi.org/10.1093/mnras/stw488

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