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Disks of classical Be stars
- 1.0124602 - ASU-R 20000058 RIV US eng C - Conference Paper (international conference)
Štefl, Stanislav
Disks of classical Be stars.
Variable and non-spherical stellar winds in luminous hot stars. Berlin: Springer, 1999 - (Wolf, B.; Fullerton, A.; Stahl, O.), s. 24-31. IAU Colloquium. 169.
[International Astronomical Union Colloquium /169./. Heidelberg (DE), 15.06.1998-19.06.1998]
R&D Projects: GA ČR GA202/97/0326
Institutional research plan: CEZ:AV0Z1003909
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
Observational methods used in investigation of circumstellar disks of Be stars significantly changed during the last decade. While mostly the studies of line profiles in the optical and near-IR region were used in the 70th and 80th, the present progress is done also thanks to interferometric and polarimetric observations.
Permanent Link: http://hdl.handle.net/11104/0022861
Number of the records: 1