- Direct N-body simulations of globular clusters-III. Palomar 4 on an eccentric orbit2017 | Faculty of Mathematics and Physics
- SPH/N-Body simulations of small (D=10 km) asteroidal breakups and improved parametric relations for Monte-Carlo collisional models2017 | Faculty of Mathematics and Physics
- Dynamical evolution of dense star clusters in galactic nuclei2014 | Faculty of Mathematics and Physics
- Clarissa Family Age from the Yarkovsky Effect Chronology2020 | Faculty of Mathematics and Physics
- The Lifetimes of Star Clusters Born with a Top-heavy IMF2020 | Faculty of Mathematics and Physics
- The violent collisional history of aqueously evolved (2) Pallas2020 | Faculty of Mathematics and Physics
- Physical and dynamical characterization of the Euphrosyne asteroid family2020 | Faculty of Mathematics and Physics
- A study of 3-dimensional shapes of asteroid families with an application to Eos2019 | Faculty of Mathematics and Physics
- The Random Walk of Cars and Their Collision Probabilities with Planets2018 | Faculty of Mathematics and Physics
- How fast is mass segregation happening in hierarchically formed embedded star clusters?2017 | Faculty of Mathematics and Physics
- BiPoS1-a computer programme for the dynamical processing of the initial binary star population2022 | Faculty of Mathematics and Physics
- Gas Expulsion in MOND: The Possible Origin of Diffuse Globular Clusters and Ultra-faint Dwarf Galaxies2018 | Faculty of Mathematics and Physics
- Complete ejection of OB stars from very young star clusters and the formation of multiple populations2019 | Faculty of Mathematics and Physics
- Stellar streams as gravitational experiments I. The case of Sagittarius2017 | Faculty of Mathematics and Physics
- THE PROPERTIES OF HYPERVELOCITY STARS AND S-STARS ORIGINATING FROM AN ECCENTRIC DISK AROUND A SUPERMASSIVE BLACK HOLE2016 | Faculty of Mathematics and Physics
- Stellar streams as gravitational experiments II. Asymmetric tails of globular cluster streams2018 | Faculty of Mathematics and Physics
- The Effect of Arm Stiffness on the Elasto-Kinematic Properties of Single-Axle Suspension by Using the MBS Simulation Model2017 | Central Library of Charles University
- Do star clusters form in a completely mass-segregated way?2019 | Faculty of Mathematics and Physics
- TOI-216: Resonant Constraints on Planet Migration2022 | Faculty of Mathematics and Physics
- Do ultracompact dwarf galaxies form monolithically or as merged star cluster complexes?2021 | Faculty of Mathematics and Physics
- THE PROPERTIES OF DYNAMICALLY EJECTED RUNAWAY AND HYPER-RUNAWAY STARS2012 | Faculty of Mathematics and Physics
- The black hole retention fraction in star clusters2018 | Faculty of Mathematics and Physics
- The distribution and morphologies of Fornax Cluster dwarf galaxies suggest they lack dark matter2022 | Faculty of Mathematics and Physics
- The bound fraction of young star clusters2017 | Faculty of Mathematics and Physics
- Evolution of globular-cluster systems of ultra-diffuse galaxies due to dynamical friction in MOND gravity2021 | Faculty of Mathematics and Physics
- Dynamics of multiple protoplanets embedded in gas and pebble discs and its dependence on Sigma and nu parameters2018 | Faculty of Mathematics and Physics