Improved encounter scenario for planetary embryos - A comparison between single-star and binary-star systems
- Author(s)
- Elke Pilat-Lohinger, Thomas Maindl, David Bancelin, Christoph Schäfer, Ákos Bazsó
- Abstract
For terrestrial planet formation the so-called perfect merging iscommonly used even if this assumption is a weak point in the formation scenario. Including results from simulations of real collisions using SPH (Smooth Particle Hydrodynamics) provide better results for the growth of planetary embryos and lead therefore to a more realistic formation scenario. The improvements due to SPH simulations will be figured out for single and binary star systems as part for comparison.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Eberhard Karls Universität Tübingen
- No. of pages
- 2
- Publication date
- 09-2018
- Austrian Fields of Science 2012
- 103003 Astronomy, 103004 Astrophysics
- Keywords
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/1da8118e-79c8-42dd-80a3-43d6259035a1