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stellar mass
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publication
Rotation curves of galaxies and the stellar mass-to-light ratio
2018 |
Matematicko-fyzikální fakulta
publication
Evolution of Accretion States in Stellar-mass Black Hole X-ray Binaries
2021 |
Matematicko-fyzikální fakulta
publication
Characterization of variability to unveil the link between pulsations and stellar mass-loss in B-Supergiants
2022 |
Matematicko-fyzikální fakulta
publication
Has JWST Already Falsified Dark-matter-driven Galaxy Formation?
2022 |
Matematicko-fyzikální fakulta
publication
The Lifetimes of Star Clusters Born with a Top-heavy IMF
2020 |
Matematicko-fyzikální fakulta
publication
The Formation of Exponential Disk Galaxies in MOND
2020 |
Matematicko-fyzikální fakulta
publication
The High Fraction of Thin Disk Galaxies Continues to Challenge ?CDM Cosmology
2022 |
Matematicko-fyzikální fakulta
publication
GK Bootis and AE Fornacis: two low-mass eclipsing binaries with dwarf companions
2012 |
Matematicko-fyzikální fakulta
publication
Simulations of star-forming main-sequence galaxies in Milgromian gravity
2023 |
Matematicko-fyzikální fakulta
publication
The most massive stars in very young star clusters with a limited mass: Evidence favours significant self-regulation in the star formation processes
2023 |
Matematicko-fyzikální fakulta
publication
Downsizing revised: Star formation timescales for elliptical galaxies with an environment-dependent IMF and a number of SNIa
2021 |
Matematicko-fyzikální fakulta
publication
Call to Adopt a Nominal Set of Astrophysical Parameters and Constants to Improve the Accuracy of Fundamental Physical Properties of Stars
2011 |
Matematicko-fyzikální fakulta
publication
The optimally sampled galaxy-wide stellar initial mass function Observational tests and the publicly available GalIMF code
2017 |
Matematicko-fyzikální fakulta
publication
X-ray polarization properties of partially ionized equatorial obscurers around accreting compact objects
2023 |
Matematicko-fyzikální fakulta
publication
Was the Milky Way a chain galaxy? Using the IGIMF theory to constrain the thin-disc star formation history and mass
2019 |
Matematicko-fyzikální fakulta
publication
Do ultracompact dwarf galaxies form monolithically or as merged star cluster complexes?
2021 |
Matematicko-fyzikální fakulta
publication
The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
2019 |
Matematicko-fyzikální fakulta
publication
Simple interpolation functions for the galaxy-wide stellar initial mass function and its effects in early-type galaxies
2019 |
Matematicko-fyzikální fakulta
publication
DYNAMICS AND TRANSIT VARIATIONS OF RESONANT EXOPLANETS
2016 |
Matematicko-fyzikální fakulta
publication
Impact of metallicity and star formation rate on the time-dependent, galaxy-wide stellar initial mass function
2018 |
Matematicko-fyzikální fakulta
publication
A Possible Solution for the M/L-[Fe/H] Relation of Globular Clusters in M31. II. The Age-Metallicity Relation
2017 |
Matematicko-fyzikální fakulta
publication
Extreme mass ratio inspirals into black holes surrounded by matter
2022 |
Matematicko-fyzikální fakulta
publication
Stellar streams as gravitational experiments I. The case of Sagittarius
2017 |
Matematicko-fyzikální fakulta
publication
Stellar streams as gravitational experiments II. Asymmetric tails of globular cluster streams
2018 |
Matematicko-fyzikální fakulta
publication
CATCH ME IF YOU CAN: IS THERE A "RUNAWAY-MASS" BLACK HOLE IN THE ORION NEBULA CLUSTER?
2012 |
Matematicko-fyzikální fakulta
publication
Generation of inclined protoplanetary discs and misaligned planets through mass accretion - I. Coplanar secondary discs
2017 |
Matematicko-fyzikální fakulta
publication
The origin of discrete multiple stellar populations in globular clusters
2017 |
Matematicko-fyzikální fakulta
publication
Very massive stars in not so massive clusters
2018 |
Matematicko-fyzikální fakulta
publication
Chemical evolution of ultra-faint dwarf galaxies in the self-consistently calculated integrated galactic IMF theory
2020 |
Matematicko-fyzikální fakulta
publication
From X-ray Binaries to Ultraluminous X-ray Sources: Evolution of Accretion Disks Across Different States with Relativistic and Non- Relativistic Disk Models
2023 |
Matematicko-fyzikální fakulta