0124680 - ASU-R 20000136 RIV DK eng C - Konferenční příspěvek (zahraniční konf.)
Baade, D. - Rivinius, T. - Štefl, Stanislav
The power of MONS for a comparative study of Be and Bn stars.
The third MONS workshop: Science preparation and target selection. Aarhus: Aarhus University Press, 2000 - (Christensen-Dalsgaard, J.; Kjeldsen, M.), s. 65-70
[Workshop on Measuring Oscillations in Nearly Stars /3./. Aarhus (DK), 24.01.2000-26.01.2000]
Výzkumný záměr: CEZ:AV0Z1003909
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika

Both Be and Bn stars are characterized by rapid rotation, but low-order g-mode nonradial pulsations were observed at least in some Be stars but not in Bn stars. Similar pulsations are observed alos in slowly pulsating B stars, which rotate on average slowly. The proposed comparative photometric MONS study of pusation properties of these stars is likely to yield the observational basis for better understanding of these processes.
Trvalý link: http://hdl.handle.net/11104/0022939