Publikace
- Directly testing gravity with Proxima Centauri2019 | 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
- Dynamical equivalence, the origin of the Galactic field stellar and binary population, and the initial radius-mass relation of embedded clusters2018 | Matematicko-fyzikální fakulta
- On the initial binary population for star cluster simulations2017 | Matematicko-fyzikální fakulta
- Using binary statistics in Taurus-Auriga to distinguish between brown dwarf formation processes2017 | 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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