0125228 - ASU-R 20030134 RIV FR eng J - Journal Article
Rivinius, Th. - Baade, D. - Štefl, Stanislav
Non-radially pulsating Be stars.
Astronomy & Astrophysics. Roč. 411, č. 2 (2003), s. 229-247. ISSN 0004-6361. E-ISSN 1432-0746
R&D Projects: GA AV ČR IAA3003001; GA MŠMT ME 531
Institutional research plan: CEZ:AV0Z1003909
Keywords : Be stars * emission line * oscillations
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
Impact factor: 3.843, year: 2003

Based on more than 3000 high-resolution echelle spectra of 27 early-type Be stars, taken over six yeras, it is shown that the short-term periodic line profile variability of these objects is due to non-radial puslation.
Permanent Link: http://hdl.handle.net/11104/0023486