I am a PhD student working in the
stellar physics group at the
Argelander Institute for Astronomy.
I am working on the main sequence evolution
of very massive stellar models, using the
binary stellar evolution code (BEC).
I produce a grid of rotating stellar evolution
models with initial masses up to 500 solarmass (LMC).
These models including a population synthesis will be used for the comparison with the VLT FLAMES Tarantula Survey.
phone: 0228-73 3390