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| Paper: |
A progress report on the search for delta Scuti pulsations of gamma Doradus candidates in the classical instability strip |
| Volume: |
256, Observational Aspects of Pulsating B and A Stars |
| Page: |
117 |
| Authors: |
Handler, G.; Shobbrook, R. R. |
| Abstract: |
The gamma Dor stars are late A/early F main-sequence stars which exhibit gravity (g)-mode pulsations with periods around one day. The delta Sct stars, on the other hand, are pressure (p)-mode pulsators with periods typically of a few hours. Despite this fundamentally different pulsational behaviour, the regions of these two classes of pulsator in the HR diagram overlap. |
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