- Moving-mesh radiation-hydrodynamic simulations of wind-reprocessed transients2021 | Faculty of Mathematics and Physics
- 3D hydrodynamic simulations for the formation of the Local Group satellite planes2022 | Faculty of Mathematics and Physics
- The Global Stability of M33 in MOND2020 | Faculty of Mathematics and Physics
- The El Gordo Galaxy Cluster Challenges ?CDM for Any Plausible Collision Velocity2023 | Faculty of Mathematics and Physics
- Fast galaxy bars continue to challenge standard cosmology2021 | Faculty of Mathematics and Physics
- Numerical modelling of gravel remobilization competence in mountain stream2014 | Faculty of Science
- Determination of Size of Molecular Clusters of Ethanol by Means of NMR Diffusometry and Hydrodynamic Calculations2014 | Faculty of Mathematics and Physics
- Kinematics of mass-loss from the outer Lagrange point L22019 | Faculty of Mathematics and Physics
- Estimating the depth of gaps opened by planets in eccentric orbit2023 | Faculty of Mathematics and Physics
- Eccentricity excitation and merging of planetary embryos heated by pebble accretion2017 | Faculty of Mathematics and Physics
- Numerical modeling of heavily polluted fine-grained sediments remobilization in northern Czech Republic2015 | Faculty of Science
- Star formation triggered by galaxy interactions in modified gravity2016 | Faculty of Mathematics and Physics
- H I mapping of the Leo Triplet Morphologies and kinematics of tails and bridges2022 | Faculty of Mathematics and Physics
- Evolution of the eccentricity and inclination of low-mass planets subjected to thermal forces: a numerical study2023 | Faculty of Mathematics and Physics
- Binary Planet Formation by Gas-assisted Encounters of Planetary Embryos2018 | Faculty of Mathematics and Physics
- The Formation of Exponential Disk Galaxies in MOND2020 | Faculty of Mathematics and Physics
- How many explosions does one need? Quantifying supernovae in globular clusters from iron abundance spreads2021 | Faculty of Mathematics and Physics
- Spreading pressure bumps in gas-dust discs can stall planet migration via planet-vortex interactions2022 | Faculty of Mathematics and Physics
- How the planetary eccentricity influences the pebble isolation mass2022 | Faculty of Mathematics and Physics
- Oscillatory migration of accreting protoplanets driven by a 3D distortion of the gas flow2019 | Faculty of Mathematics and Physics
- Three-dimensional simulations of clump formation in stellar wind collisions2020 | Faculty of Mathematics and Physics
- Stellar Winds Pump the Heart of the Milky Way2020 | Faculty of Mathematics and Physics
- On the absence of backsplash analogues to NGC 3109 in the Lambda CDM framework2021 | Faculty of Mathematics and Physics
- TOI-216: Resonant Constraints on Planet Migration2022 | Faculty of Mathematics and Physics
- Supernovae in colliding-wind binaries: observational signatures in the first year2022 | Faculty of Mathematics and Physics
- How fast do young star clusters expel their natal gas? Estimating the upper limit of the gas expulsion time-scale2020 | Faculty of Mathematics and Physics
- A massive blow for ACDM - the high redshift, mass, and collision velocity of the interacting galaxy cluster El Gordo contradicts concordance cosmology2021 | Faculty of Mathematics and Physics
- Post-dynamical inspiral phase of common envelope evolution Binary orbit evolution and angular momentum transport2023 | Faculty of Mathematics and Physics
- Supernova explosions interacting with aspherical circumstellar material: implications for light curves, spectral line profiles, and polarization2020 | Faculty of Mathematics and Physics
- Migration of gap-opening planets in 3D stellar-irradiated accretion disks2020 | Faculty of Mathematics and Physics