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stars:abundances
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How many explosions does one need? Quantifying supernovae in globular clusters from iron abundance spreads
2021 |
Faculty of Mathematics and Physics
publication
The giants that were born swiftly - implications of the top-heavy stellar initial mass function on the birth conditions of globular clusters
2022 |
Faculty of Mathematics and Physics
publication
PHOTODETACHMENT AS A DESTRUCTION MECHANISM FOR CN- AND C3N- ANIONS IN CIRCUMSTELLAR ENVELOPES
2013 |
Faculty of Mathematics and Physics
publication
The effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history
2020 |
Faculty of Mathematics and Physics
publication
Chemical cartography of the Milky Way
2023 |
Faculty of Mathematics and Physics
publication
The convective kissing instability in low-mass M-dwarf models: convective overshooting, semi-convection, luminosity functions, surface abundances, and star cluster age dating
2023 |
Faculty of Mathematics and Physics