Publikace
- Was the Milky Way a chain galaxy? Using the IGIMF theory to constrain the thin-disc star formation history and mass2019 | Matematicko-fyzikální fakulta
- Rotation curves of galaxies and the stellar mass-to-light ratio2018 | Matematicko-fyzikální fakulta
- Star formation in the outskirts of DDO 154: a top-light IMF in a nearly dormant disc2018 | Matematicko-fyzikální fakulta
- On the origin of the Schechter-like mass function of young star clusters in disc galaxies2017 | Matematicko-fyzikální fakulta
- Generation of inclined protoplanetary discs and misaligned planets through mass accretion - I. Coplanar secondary discs2017 | Matematicko-fyzikální fakulta
- Simulations of star-forming main-sequence galaxies in Milgromian gravity2023 | 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
- Hydrodynamical structure formation in Milgromian cosmology2023 | Matematicko-fyzikální fakulta
- Degree of stochastic asymmetry in the tidal tails of star clusters2023 | Matematicko-fyzikální fakulta
- The cosmological star formation history from the Local Cosmological Volume of galaxies and constraints on the matter homogeneity2023 | Matematicko-fyzikální fakulta
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