Katerina Magg

Previous

PhD student
(*former Semenova)

Interests

Stellar physics, photometry, spectral analysis
Physical processes in stellar interior (gravitational settling, rotation, mixing)
3D Non-LTE studies of heavy elements 

PhD 
Analysis of the effects of diffusion and gravitational setting using the Gaia-ESO observations of open clusters
Fe-group elements in galactic populations

Papers
Observational constraints on the origin of the elements. IV: The standard composition of the Sun
Magg, Bergemann, Serenelli et al. A&A, 661, id.A140, 2022
Press release:
 https://www.mpia.de/5857710/news_publication_18652392_transferred

"The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing at the origin of chemical abundance variations”
Semenova, Bergemann, Deal, incl. Hansen et al., A&A, 643, id.A164, 2020



© Maria Bergemann 2023