Workshop :
"Physics of Stellar Winds and Circumstellar Disks"
Tuesday, September 13, 2011
Seminar Room, Ondřejov
(former computer center)
Program
| 09:30 - 10:00 | COFFEE | |||||
| Session I | Stellar evolution, stellar winds and mass loss | |||||
| 10:00 - 10:50 | The Circumstellar Environment of Rotating Stars: | Anahi Granada | Geneva Observatory | |||
| Near IR Spectroscopy of Be Stars, Slow Radiation- | ||||||
| Driven Wind Solutions of A-type Supergiants and | ||||||
| Stellar Evolution Modeling of Rapidly Rotating Stars. | ||||||
| 10:50 - 11:30 | 3D Monte Carlo Radiative Transfer in Hot Star Winds | Brankica Šurlan | Astronomický ústav Ondřejov | |||
| 11:30 - 13:00 | LUNCH | |||||
| 13:00 - 14:00 | Massive Star Winds and their Circumstellar Disks | Asif ud-Doula | Penn State Worthington Scranton | |||
| 14:00 - 14:50 | Hot star wind mass-loss rates: theory versus | Jiří Krtička | PřF MU Brno | |||
| observations | ||||||
| 14:50 - 15:20 | COFFEE BREAK | |||||
| Session II | B[e] stars, supergiants, and circumstellar disks | |||||
| 15:20 - 16:10 | On the evolutionary stage and the disk formation | Florencia Muratore | Instituto de Astrofísica de La Plata | |||
| mechanism of B[e] supergiants | ||||||
| 16:10 - 16:45 | Detection of Raman scattered emission lines in | Andrea Torres | Instituto de Astrofísica de La Plata | |||
| the B[e] supergiant LHA 115-S 18 | ||||||
| 16:45 - 17:10 | Line driven winds of rapidly rotating hot stars: Is it | Michal Ceniga | PřF MU Brno | |||
| enough for the explanation of B[e] stars' disks? | ||||||
| 17:10 - 17:45 | Decretion disks of rapidly rotating hot stars | Petr Kurfürst | PřF MU Brno | |||
| 19:00 | SOCIAL EVENT | |||||