Katerina Semenova

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PhD student

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

Papers
"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., submitted to the GES collaboration for internal review 



© Maria Bergemann 2019