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@proceedings{1075366, author = {Šejnová, Klára and Votruba, Viktor and Koubský, Pavel}, booktitle = {Circumstellar Dynamics at High Resolution}, keywords = {Be stars shellspec genetic algorithms}, language = {eng}, isbn = {978-1-58381-810-7}, title = {Modeling of Be Stars}, year = {2012} }
TY - CONF ID - 1075366 AU - Šejnová, Klára - Votruba, Viktor - Koubský, Pavel PY - 2012 TI - Modeling of Be Stars SN - 9781583818107 KW - Be stars shellspec genetic algorithms N2 - 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. ER -
ŠEJNOVÁ, Klára, Viktor VOTRUBA a Pavel KOUBSKÝ. Modeling of Be Stars. In \textit{Circumstellar Dynamics at High Resolution}. 2012. ISBN~978-1-58381-810-7.
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