Gravity-dominated Collisions: A Model for the Largest Remnant Masses with Treatment for “Hit and Run” and Density Stratification

We develop empirical relationships for the accretion and erosion of colliding gravity-dominated bodies of various compositions under conditions expected in late-stage solar system formation. These are fast, easily coded relationships based on a large database of smoothed particle hydrodynamics (SPH)...

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Detalles Bibliográficos
Autores principales: Gabriel, Travis S. J., Jackson, Alan P., Asphaug, Erik, Reufer, Andreas, Jutzi, Martin, Benz, Willy
Formato: Online Artículo Texto
Lenguaje:English
Publicado: 2020
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8097937/
https://www.ncbi.nlm.nih.gov/pubmed/33958809
http://dx.doi.org/10.3847/1538-4357/ab528d

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8097937/
https://www.ncbi.nlm.nih.gov/pubmed/33958809
http://dx.doi.org/10.3847/1538-4357/ab528d

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