241 citations · 2.3k across the 71 of their papers we have counts for
7 papers · 1 filter
Short dissipation times of proto-planetary discs - an artifact of selection effects?
Susanne Pfalzner, Manuel Steinhausen, Karl Menten
The frequency of discs around young stars, a key parameter for understanding planet formation, is most readily determined in young stellar clusters where many relatively coeval sta…
The evolutionary tracks of young massive star clusters
S. Pfalzner, G. Parmentier, M. Steinhausen +2
Stars mostly form in groups consisting of a few dozen to several ten thousand members. For 30 years, theoretical models provide a basic concept of how such star clusters form and d…
Stellar age spreads in clusters as imprints of cluster-parent clump densities
Genevieve Parmentier, Susanne Pfalzner, Eva K. Grebel
It has recently been suggested that high-density clusters have stellar age distributions narrower than that of the Orion Nebula Cluster, indicating a possible trend of narrower age…
ATLASGAL --- towards a complete sample of massive star forming clumps
J. S. Urquhart, T. J. T. Moore, T. Csengeri +12
By matching infrared-selected, massive young stellar objects (MYSOs) and compact HII regions in the RMS survey to massive clumps found in the submillimetre ATLASGAL survey, we have…
Revisiting the universality of (multiple) star formation in present-day star formation regions
Michael Marks, Nathan Leigh, Mirek Giersz +3
Populations of multiple stars inside clustered regions are known to change through dynamical interactions. The efficiency of binary disruption is thought to be determined by stella…
Sizes of protoplanetary discs after star-disc encounters
Andreas Breslau, Manuel Steinhausen, Kirsten Vincke +1
Most stars do not form in isolation, but as part of a star cluster or association. These young stars are initially surrounded by protoplanetary discs. In these cluster environments…