activity
20052015
most citedFrom dust to planetesimals: an improved model for collisional growth in protoplanetary disks

131 citations · 710 across the 17 of their papers we have counts for

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Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2015★ 13 cited

GalevNB: a conversion from N-BODY simulations to observations

Xiaoying Pang, Christoph Olczak, Difeng Guo +2

We present (Galev for -body simulations), an utility that converts fundamental stellar properties of -body simulations into observational properties using the $GALE…

astro-ph.GA2015

GalevNB: Galev for N-Body simulations

Xiaoying Pang, Christoph Olczak, Rainer Spurzem

We report on GalevNB (Galev for N-Body simulations), an integrated software solution that provides N-body users direct access to the software package GALEV (GALaxy EVolutionary syn…

astro-ph.GA2015★ 66 cited

On the occurrence of galaxy harassment

Daniel Bialas, Thorsten Lisker, Christoph Olczak +2

Tidal interactions of galaxies in galaxy clusters have been proposed as one potential explanation of the morphology-density relation at low masses. The efficiency of tidal transfor…

astro-ph.GA2012★ 26 cited

Modes of clustered star formation

S. Pfalzner, T. Kaczmarek, C. Olczak

The realization that most stars form in clusters, raises the question of whether star/planet formation are influenced by the cluster environment. The stellar density in the most pr…

astro-ph.GA2012★ 42 cited

The Evolution of Protoplanetary Disks in the Arches Cluster

C. Olczak, T. Kaczmarek, S. Harfst +2

Most stars form in a cluster environment. These stars are initially surrounded by discs from which potentially planetary systems form. Of all cluster environments starburst cluster…

astro-ph.GA2011★ 41 cited

Simulations of the Hyades

A. Ernst, A. Just, P. Berczik +1

Context: Using the recent observational data of Röser et al. we present -body simulations of the Hyades open cluster. Aims: We make an attempt to determine initial conditions of…