Publikace
- MOND simulation suggests an origin for some peculiarities in the Local Group2018 | 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
- The El Gordo Galaxy Cluster Challenges ?CDM for Any Plausible Collision Velocity2023 | Matematicko-fyzikální fakulta
- The convective kissing instability in low-mass M-dwarf models: convective overshooting, semi-convection, luminosity functions, surface abundances, and star cluster age dating2023 | Matematicko-fyzikální fakulta
- The integrated galaxy-wide stellar initial mass function over the radial acceleration range of early-type galaxies2023 | Matematicko-fyzikální fakulta
- A simultaneous solution to the Hubble tension and observed bulk flow within 250 h -1 Mpc2023 | Matematicko-fyzikální fakulta
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