A progress report on the search for delta Scuti pulsations of gamma Doradus candidates in the classical instability strip

Details A progress report on the search for delta Scuti pulsations of gamma Doradus candidates in the classical instability strip A progress report on the search for delta Scuti pulsations of gamma Doradus candidates in the classical instability strip

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..256..117h&link_type=abstract

Observational Aspects of Pulsating B- and A Stars, ASP Conference Proceedings, Vol. 256. Edited by Christiaan Sterken and Donal

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Scientific paper

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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