Dissipative N-body & gasodynamical model of the triaxial protogalaxy collapse
- Author(s)
- P. P. Berczik, S. G. Kravchuk, R. Spurzem, G. Hensler
- Abstract
This work is devoted to the study of complex modelling of formation and
evolution of galaxies and galactic structures using multivariate methods
of numerical simulations based on particles methods (the N-body
problem). Multi-dimensional gas-dynamics calculations were carried out
in the work with a particle-based method, namely SPH - Smoothed Particle
Hydrodynamics. In this work a newly developed Chemo-Dynamical Smoothed
Particle Hydrodynamics (CD-SPH) code is presented.
- Organisation(s)
- Department of Astrophysics
- Journal
- Dark energy and dark matter in the Universe: in three volumes
- Pages
- 191-293
- Publication date
- 2014
- Austrian Fields of Science 2012
- 103004 Astrophysics
- Keywords
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/0ba9b51a-3f85-4e07-87f6-d1ea5b2244e4