Classes
Publications
- Variable line profiles due to non-axisymmetric patterns in an accretion disc around a rotating black hole2001 | Faculty of Mathematics and Physics
- Estimating the Ages of Open Star Clusters from Properties of Their Extended Tidal Tails2022 | Faculty of Mathematics and Physics
- The giants that were born swiftly - implications of the top-heavy stellar initial mass function on the birth conditions of globular clusters2022 | Faculty of Mathematics and Physics
- Asymmetrical tidal tails of open star clusters: stars crossing their cluster's prah(dagger) challenge Newtonian gravitation2022 | Faculty of Mathematics and Physics
- How many explosions does one need? Quantifying supernovae in globular clusters from iron abundance spreads2021 | Faculty of Mathematics and Physics
- Enhanced Kozai-Lidov Eccentricity Oscillations in Nuclear Star Clusters2021 | Faculty of Mathematics and Physics
- Very high redshift quasars and the rapid emergence of supermassive black holes2020 | Faculty of Mathematics and Physics
- Intermediate-mass black holes in binary-rich star clusters2019 | Faculty of Mathematics and Physics
- Do star clusters form in a completely mass-segregated way?2019 | Faculty of Mathematics and Physics
- The hunt for self-similar core collapse2018 | Faculty of Mathematics and Physics
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