- Active Hot Stars including, Be, B[e], WR, O and LBV stars.
- Mass loss around hot stars
- Stellar winds
- Models (development of the SIMECA code)
- Non-LTE Radiative Transfer
- Hydrodynamics
- High angular resolution and large baseline optical interferometry
- Project Scientist of the VEGA/CHARA interferometer
- Exploitation of the AMBER and MIDI instruments on the VLTI
UMR LAGRANGE
Observatoire de la Côte d’Azur
Boulevard de l’Observatoire
CS 34229 - F 06304 NICE Cedex 4
Tél. : +33 (0)4 92 00 30 11
Fax : +33 (0)4 92 00 30 33