Předměty
Publikace
- THE PROPERTIES OF DYNAMICALLY EJECTED RUNAWAY AND HYPER-RUNAWAY STARS2012 | Matematicko-fyzikální fakulta
- A toy model for star-disc collisions2000 | Matematicko-fyzikální fakulta
- Estimating the Ages of Open Star Clusters from Properties of Their Extended Tidal Tails2022 | Matematicko-fyzikální fakulta
- The giants that were born swiftly - implications of the top-heavy stellar initial mass function on the birth conditions of globular clusters2022 | Matematicko-fyzikální fakulta
- Asymmetrical tidal tails of open star clusters: stars crossing their cluster's prah(dagger) challenge Newtonian gravitation2022 | Matematicko-fyzikální fakulta
- How many explosions does one need? Quantifying supernovae in globular clusters from iron abundance spreads2021 | Matematicko-fyzikální fakulta
- Enhanced Kozai-Lidov Eccentricity Oscillations in Nuclear Star Clusters2021 | Matematicko-fyzikální fakulta
- Very high redshift quasars and the rapid emergence of supermassive black holes2020 | Matematicko-fyzikální fakulta
- Intermediate-mass black holes in binary-rich star clusters2019 | Matematicko-fyzikální fakulta
- Do star clusters form in a completely mass-segregated way?2019 | Matematicko-fyzikální fakulta
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