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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.
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