- The origin and orbit of the old, metal-rich, open cluster NGC 6791 Insights from kinematics2012 | Matematicko-fyzikální fakulta
- Tidal tails of open star clusters as probes to early gas expulsion: II. Predictions for Gaia2020 | Matematicko-fyzikální fakulta
- A sextet of clusters in the Vela OB2 region revealed by Gaia2018 | Matematicko-fyzikální fakulta
- Very massive stars in not so massive clusters2018 | Matematicko-fyzikální fakulta
- Gaia Early Data Release 3 The Galactic anticentre2021 | Matematicko-fyzikální fakulta
- Tidal tails of open star clusters as probes of early gas expulsion: I. A semi-analytic model2020 | Matematicko-fyzikální fakulta
- Uncovering a 260 pc wide, 35-Myr-old filamentary relic of star formation2020 | Matematicko-fyzikální fakulta
- On the initial binary population for star cluster simulations2017 | Matematicko-fyzikální fakulta
- Dynamical equivalence, the origin of the Galactic field stellar and binary population, and the initial radius-mass relation of embedded clusters2018 | Matematicko-fyzikální fakulta
- A stellar relic filament in the Orion star-forming region2019 | Matematicko-fyzikální fakulta
- On the dynamical evolution of Cepheids in star clusters & x22c6;2022 | Matematicko-fyzikální fakulta
- Dynamical equivalence, the origin of the Galactic field stellar and binary population, and the initial radius-mass relation of embedded clusters (vol 474, pg 3740, 2018)2019 | Matematicko-fyzikální fakulta
- How fast do young star clusters expel their natal gas? Estimating the upper limit of the gas expulsion time-scale2020 | Matematicko-fyzikální fakulta
- Degree of stochastic asymmetry in the tidal tails of star clusters2023 | Matematicko-fyzikální fakulta
- Evidence for feedback and stellar-dynamically regulated bursty star cluster formation: the case of the Orion Nebula Cluster2018 | Matematicko-fyzikální fakulta, Ústřední knihovna
- When the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster2019 | Matematicko-fyzikální fakulta
- The most massive stars in very young star clusters with a limited mass: Evidence favours significant self-regulation in the star formation processes2023 | Matematicko-fyzikální fakulta
- Asymmetrical tidal tails of open star clusters: stars crossing their cluster's prah(dagger) challenge Newtonian gravitation2022 | Matematicko-fyzikální fakulta