Discovery of the `missing' mode in HR1217 by the Whole Earth Telescope
HR1217 is a prototypical rapidly oscillating Ap star that has presented a test to the theory of non-radial stellar pulsation. Prior observations showed a clear pattern of five modes with alternating frequency spacings of 33.3 and 34.6μHz, with a sixth mode at a problematic spacing of 50.0μHz (which equals to the high-frequency side. Asymptotic
Kurtz, D. W. et al.
Fecha de publicación:
3
2002