PhD student
Interests
3D radition-hydrodynamical models of stellar atmospheres and diagnostic spectroscopy
Chemical evolution of the Milky Way
Physics and progenitors of SN Ia
Recent papers
M3DIS - A grid of 3D radiation-hydrodynamics stellar atmosphere models for stellar surveys. I. Procedure, validation, and the Sun
Eitner, Bergemann, Hoppe et al., A&A, 688, A52, 2024
Observational constraints on the origin of the elements. V. Constraints on the chemical enrichment by sub-Chandrasekhar mass SNe in the Milky Way
Eitner, Bergemann, Ruiter et al., A&A, 677, A151, 2023
Observational constraints on the origin of the elements. III. Evidence for the dominant role of sub-Chandrasekhar SN Ia in the chemical evolution of Mn and Fe in the Galaxy
Eitner, Bergemann, Hansen et al. A&A, 635, A38, 2020
NLTE modelling of integrated light spectra. Abundances of barium, magnesium, and manganese in a metal-poor globular cluster
Eitner, Bergemann, & Larsen A&A, 627, A40