Publication details

Modeling of Be Stars

Title in English Modeling of the Be Stars
Authors

ŠEJNOVÁ Klára VOTRUBA Viktor KOUBSKÝ Pavel

Year of publication 2012
Type Appeared in Conference without Proceedings
MU Faculty or unit

Faculty of Science

Citation
Description 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.

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