| |
 |
| Paper: |
Modeling of Be Stars |
| Volume: |
464, Circumstellar Dynamics at High Resolution |
| Page: |
219 |
| Authors: |
Šejnová, K.; Votruba, V.; Koubská, P. |
| Abstract: |
Be stars are still a big unknown in respect of origin and geometry of
circumstellar disk around a star. The program shellspec is designed
to solve a simple radiative transfer along the line of sight in
three-dimensional moving media, so it is able to compute synthetic spectrum
for our case (a star with a disk). Our goal was to develop an effective
method to search in parameter space which can allow us to find a good estimate
of physical parameters of the disk. |
|
|
|
|
|
