|
Time-resolved high-resolution spectroscopy of the pulsating sdB star QQ Vir (PG1325+101) John Telting et al., Shanghai, July 2009 |
|
||||||||
|
|
|
||||||||||||
The pulsating β Cephei star ω Sco, rotational
velocity Vsin(i)= 100 km/s, Vmag =
3.9 with main mode L = |M| = 9 (Berdyugina et al. 2003)
About 50% of stars with spectral type in the β Cep domain show wiggles in their line profiles (Telting et al. 2006).