Deutsch Intern
  • "Eta-Catarina-Nebula"

Niklas Bauer

Master Student

Building: 31 (Physik Ost)
Room: 01.009

Goal: Estimation of the gamma-ray flux from decaying Al-26 (1809 keV) and Fe-60 (1.173, 1332 keV) from recent supernovae (3–6 Myr ago) inside the Local Bubble.

Methods: Spatial modelling, line-of-sight integration (discrete and Monte Carlo), stellar evolution yields (as a function of mass, metallicity, rotation), data simulations (COSI SMEX).

Link to Bachelor thesis: Link