0125228 - ASU-R 20030134 RIV FR eng J - Článek v odborném periodiku
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
Grant CEP: GA AV ČR IAA3003001; GA MŠMT ME 531
Výzkumný záměr: CEZ:AV0Z1003909
Klíčová slova: Be stars * emission line * oscillations
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 3.843, rok: 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.
Trvalý link: http://hdl.handle.net/11104/0023486