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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...
| Autores principales: | , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Oxford University Press
2016
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| 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 |