Dissipative N-body & gasodynamical model of the triaxial protogalaxy collapse

Autor(en)

P. P. Berczik, S. G. Kravchuk, R. Spurzem, G. Hensler

Abstrakt

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(en)

Institut für Astrophysik

Journal

Dark energy and dark matter in the Universe: in three volumes

Seiten

191-293

Publikationsdatum

2014

ÖFOS 2012

103004 Astrophysik

Schlagwörter

Link zum Portal

Dissipative N-body &amp; gasodynamical model of the triaxial protogalaxy collapse