Orbit-based dynamical models of the Sculptor dSph galaxy
We have developed spherically symmetric dynamical models of dwarf spheroidal (dSph) galaxies using Schwarzschild's orbit superposition method. This type of modelling yields constraints both on the total mass distribution (e.g. enclosed mass and scale radius) and on the orbital structure of the system (e.g. velocity anisotropy). This method is thus
Breddels, Maarten A. et al.
Fecha de publicación:
8
2013