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
- The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology2019 | Matematicko-fyzikální fakulta
- Stellar streams as gravitational experiments II. Asymmetric tails of globular cluster streams2018 | Matematicko-fyzikální fakulta
- Rotation curves of galaxies and the stellar mass-to-light ratio2018 | Matematicko-fyzikální fakulta
- Very massive stars in not so massive clusters2018 | Matematicko-fyzikální fakulta
- Impact of metallicity and star formation rate on the time-dependent, galaxy-wide stellar initial mass function2018 | Matematicko-fyzikální fakulta
- Direct N-body simulations of globular clusters-III. Palomar 4 on an eccentric orbit2017 | Matematicko-fyzikální fakulta
- A Possible Solution for the M/L-[Fe/H] Relation of Globular Clusters in M31. II. The Age-Metallicity Relation2017 | Matematicko-fyzikální fakulta
- The optimally sampled galaxy-wide stellar initial mass function Observational tests and the publicly available GalIMF code2017 | Matematicko-fyzikální fakulta
- Stellar streams as gravitational experiments I. The case of Sagittarius2017 | Matematicko-fyzikální fakulta
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