activity
20242026
collaborators

6 papers

astro-ph.GA2026

Statistical study for binary star evolution in dense embedded clusters

Wenjie Wu, Pavel Kroupa, Vikrant V. Jadhav

Context: The dynamical evolution of binary populations in embedded star clusters shapes the statistical properties of binaries observed in the Galactic field. Accurately modelling…

astro-ph.GA2025

Tidal Tails of Nearby Open Clusters. II. A Review of Simulated Properties and the Reliability of Observational Catalogues

Vikrant V. Jadhav, Dhanraj Risbud, Pavel Kroupa +1

Context: Recent studies using Gaia data have reported tidal tail detections for tens to hundreds of open clusters. However, a comprehensive assessment of the reliability & complete…

astro-ph.GA2024

The evolution of the mass--radius relation of expanding very young star clusters

Jian-Wen Zhou, Pavel Kroupa, Wenjie Wu

The initial mass--radius relation of embedded star clusters is an essentially important boundary condition for understanding the evolution of embedded clusters in which stars form…

astro-ph.GA2024

Open star clusters and their asymmetrical tidal tails

Pavel Kroupa, Jan Pflamm-Altenburg, Sergij Mazurenko +4

Stars that evaporate from their star cluster by the energy equipartition process end up either in a leading or a trailing tidal tail. In Newtonian gravitation and for open star clu…

astro-ph.GA2024

Mass segregation and velocity dispersion as evidence for a dark star cluster

Wenjie Wu, Pavel Kroupa, Jan Pflamm-Altenburg

A dark star cluster (DSC) is a system in which the cluster potential is dominated by stellar remnants, such as black holes and neutron stars having larger masses than the long-live…

astro-ph.GA2024

The spin, expansion and contraction of open star clusters

Vikrant V. Jadhav, Pavel Kroupa, Wenjie Wu +2

Empirical constraints on the internal dynamics of open clusters are important for understanding their evolution and evaporation. High precision astrometry from Gaia DR3 are thus us…