- Rotation curves of galaxies and the stellar mass-to-light ratio2018 | Faculty of Mathematics and Physics
- Evolution of Accretion States in Stellar-mass Black Hole X-ray Binaries2021 | Faculty of Mathematics and Physics
- Characterization of variability to unveil the link between pulsations and stellar mass-loss in B-Supergiants2022 | Faculty of Mathematics and Physics
- Has JWST Already Falsified Dark-matter-driven Galaxy Formation?2022 | Faculty of Mathematics and Physics
- The Lifetimes of Star Clusters Born with a Top-heavy IMF2020 | Faculty of Mathematics and Physics
- The Formation of Exponential Disk Galaxies in MOND2020 | Faculty of Mathematics and Physics
- The High Fraction of Thin Disk Galaxies Continues to Challenge ?CDM Cosmology2022 | Faculty of Mathematics and Physics
- GK Bootis and AE Fornacis: two low-mass eclipsing binaries with dwarf companions2012 | Faculty of Mathematics and Physics
- Simulations of star-forming main-sequence galaxies in Milgromian gravity2023 | Faculty of Mathematics and Physics
- The most massive stars in very young star clusters with a limited mass: Evidence favours significant self-regulation in the star formation processes2023 | Faculty of Mathematics and Physics
- Downsizing revised: Star formation timescales for elliptical galaxies with an environment-dependent IMF and a number of SNIa2021 | Faculty of Mathematics and Physics
- Call to Adopt a Nominal Set of Astrophysical Parameters and Constants to Improve the Accuracy of Fundamental Physical Properties of Stars2011 | Faculty of Mathematics and Physics
- The optimally sampled galaxy-wide stellar initial mass function Observational tests and the publicly available GalIMF code2017 | Faculty of Mathematics and Physics
- X-ray polarization properties of partially ionized equatorial obscurers around accreting compact objects2023 | Faculty of Mathematics and Physics
- Was the Milky Way a chain galaxy? Using the IGIMF theory to constrain the thin-disc star formation history and mass2019 | Faculty of Mathematics and Physics
- Do ultracompact dwarf galaxies form monolithically or as merged star cluster complexes?2021 | Faculty of Mathematics and Physics
- The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology2019 | Faculty of Mathematics and Physics
- Simple interpolation functions for the galaxy-wide stellar initial mass function and its effects in early-type galaxies2019 | Faculty of Mathematics and Physics
- DYNAMICS AND TRANSIT VARIATIONS OF RESONANT EXOPLANETS2016 | Faculty of Mathematics and Physics
- Impact of metallicity and star formation rate on the time-dependent, galaxy-wide stellar initial mass function2018 | Faculty of Mathematics and Physics
- A Possible Solution for the M/L-[Fe/H] Relation of Globular Clusters in M31. II. The Age-Metallicity Relation2017 | Faculty of Mathematics and Physics
- Extreme mass ratio inspirals into black holes surrounded by matter2022 | Faculty of Mathematics and Physics
- Stellar streams as gravitational experiments I. The case of Sagittarius2017 | Faculty of Mathematics and Physics
- Stellar streams as gravitational experiments II. Asymmetric tails of globular cluster streams2018 | Faculty of Mathematics and Physics
- CATCH ME IF YOU CAN: IS THERE A "RUNAWAY-MASS" BLACK HOLE IN THE ORION NEBULA CLUSTER?2012 | Faculty of Mathematics and Physics
- Generation of inclined protoplanetary discs and misaligned planets through mass accretion - I. Coplanar secondary discs2017 | Faculty of Mathematics and Physics
- The origin of discrete multiple stellar populations in globular clusters2017 | Faculty of Mathematics and Physics
- Very massive stars in not so massive clusters2018 | Faculty of Mathematics and Physics
- Chemical evolution of ultra-faint dwarf galaxies in the self-consistently calculated integrated galactic IMF theory2020 | Faculty of Mathematics and Physics
- From X-ray Binaries to Ultraluminous X-ray Sources: Evolution of Accretion Disks Across Different States with Relativistic and Non- Relativistic Disk Models2023 | Faculty of Mathematics and Physics