Dynamical Evolution of the Disk of the Be Star 60 Cygni

0470523 - ASÚ 2018 RIV US eng C - Conference Paper (international conference)
Šejnová, K. - Votruba, Viktor - Koubský, Pavel
Dynamical Evolution of the Disk of the Be Star 60 Cygni.
Bright Emissaries: Be Stars as Messengers of Star-Disk Physics. San Francisco: Astronomical Society of the Pacific, 2016, s. 279-282. ASP Conference Series, 506. ISBN 9781583818961.
[Bright Emissaries: Be Stars as Messengers of Star-Disk Physics. Ontario (CA), 11.08.2014-13.08.2014]
Institutional support: RVO:67985815
Keywords : Be star * 60 Cygni * modeling of the disk
OECD category: Astronomy (including astrophysics,space science)

The Be stars are still very unknown in respect of origin and geometry of circumstellar disk around a star. We present here the first results of the modeling of the disk of the Be star 60 Cygni with applying modified version of the Shellspec code (Budaj & Richards 2004), which is designed to solve simple radiative transfer along the line of sight in 3D moving media. Our goal was to estimate some physical parameters of the disk, like outer radius, from observed spectra. We present here results for 60 Cygni and its disk evolution (evolution of the outer radius, opening angle, etc.) between years 2003 and 2011.
Permanent Link: http://hdl.handle.net/11104/0276785