Publikace
- On the dynamical evolution of Cepheids in star clusters & x22c6;2022 | Matematicko-fyzikální fakulta
- Estimating the Ages of Open Star Clusters from Properties of Their Extended Tidal Tails2022 | Matematicko-fyzikální fakulta
- Do the majority of stars form as gravitationally unbound?2022 | Matematicko-fyzikální fakulta
- 3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR3: Its Relation to Cluster Dynamics2021 | Matematicko-fyzikální fakulta
- SILCC VI - Multiphase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionizing radiation, and cosmic rays2021 | Matematicko-fyzikální fakulta
- Tree-based solvers for adaptive mesh refinement code flash - II: radiation transport module TreeRay2021 | Matematicko-fyzikální fakulta
- Tidal tails of open star clusters as probes to early gas expulsion: II. Predictions for Gaia2020 | Matematicko-fyzikální fakulta
- Tidal tails of open star clusters as probes of early gas expulsion: I. A semi-analytic model2020 | 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
- Evidence for feedback and stellar-dynamically regulated bursty star cluster formation: the case of the Orion Nebula Cluster2018 | Matematicko-fyzikální fakulta, Ústřední knihovna
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