activity
20052007
most cited2-Dimensional Kinematics of Simulated Disc Merger Remnants

136 citations · 266 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph200769 cited

SAURON's Challenge for the Major Merger Scenario of Elliptical Galaxy Formation

Andreas Burkert, Thorsten Naab, Peter H. Johansson

The intrinsic anisotropy delta and flattening epsilon of simulated merger remnants is compared with elliptical galaxies that have been observed by the SAURON collaboration, and tha…

astro-ph2007

Formation and evolution of galactic spheroids by mergers

Thorsten Naab, Andreas Burkert, Peter H. Johansson +1

Galactic spheroids can form as a result of galaxy interactions and mergers of disks. Detailed analyses of the photometric properties, the intrinsic orbital structure, the line-of-s…

astro-ph200757 cited

Axisymmetric orbit models of N-body merger remnants: a dependency of reconstructed mass on viewing angle

J. Thomas, R. Jesseit, T. Naab +3

We model mock observations of collisionless N-body disc-disc mergers with an axisymmetric orbit superposition program that has been used to model Coma ellipticals. The remnants sam…

astro-ph20074 cited

Influence of Orbital Behaviour and Chaos on the Shape of Dark Matter Halos

Andrea V. Maccio', Ioannis Sideris, Marco Miranda +2

It has been shown that the dissipative gas infall during galaxy formation has the capability to modify the shape of dark matter halos. In this paper we perform the first detailed a…

astro-ph2006136 cited

2-Dimensional Kinematics of Simulated Disc Merger Remnants

Roland Jesseit, Thorsten Naab, Reynier Peletier +1

We present a two-dimensional kinematic analysis for a sample of simulated binary disc merger remnants with mass ratios 1:1 and 3:1. For the progenitor discs we used pure stellar mo…

astro-ph2005

Orbital Structure of Collisionless Merger Remnants: On the Origin of Photometric and Kinematic Properties of Elliptical and S0 Galaxies

R. Jesseit, T. Naab, A. Burkert

We present a detailed investigation of the relation between the orbital content of merger remnants and observable properties of elliptical and S0 galaxies. Our analysis is based on…