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Modeling of the Be Stars
- 1.0388402 - ASÚ 2013 RIV GB eng C - Conference Paper (international conference)
Šejnová, Klára - Votruba, Viktor - Koubský, Pavel
Modeling of the Be Stars.
From Interacting Binaries to Exoplanets: Essential Modeling Tools. Cambridge: Cambridge University Press, 2012 - (Richards, M.), s. 261-262. Proceedings of the International Astronomical Union, IAU S282. ISBN 9781107019829. ISSN 1743-9213.
[Symposium of the International Astronomical Union /282./. Tatranská Lomnica (SK), 18.07.2011-22.07. 2011]
Institutional support: RVO:67985815
Keywords : Be stars * shellspec * genetic algorithms
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
The Be stars are still a big unknown in respect to the origin and geometry of the circumstellar disk around the star. Program shellspec is designed to solve the simple radiative transfer along the line of sight in three-dimensional moving media. Our goal was to develop an effective method to search in parameter space, which can allow us to find a good estimate of the physical parameters of the disk. We also present here our results for Be star 60 Cyg using the modified code.
Permanent Link: http://hdl.handle.net/11104/0217296
Number of the records: 1