|
|
Paper: |
g-Mode Pulsators along the Horizontal Branch |
Volume: |
452, Fifth Meeting on Hot Subdwarf Stars and Related Objects |
Page: |
251 |
Authors: |
O'Toole, S. J. |
Abstract: |
Kepler has been a boon for asteroseismology, detecting oscillations in
many different stars across the HR diagram. High precision data over
long timescales has allowed us to detect many
g-mode oscillations in sdB stars in particular, but also in other
Horizontal Branch stars. Here I point out the very similar g-mode
period spacings detected in sdB and Red Clump stars, and discuss what
we can learn by comparing oscillations in these objects. |
|
|
|
|