The occurrence of non-pulsating stars in the γ Dor and δ Sct instability regions. Issue Volume 9:Issue S301(2013) (18th February 2014)

• Record Type: Journal Article
• Authors: Guzik, Joyce A.; Bradley, Paul A.; Jackiewicz, Jason; Uytterhoeven, Katrien; Kinemuchi, Karen
• Is Part Of: Proceedings of the International Astronomical Union. Volume 9:Issue S301(2013)
• Page Start: 63
• Page End: 66
• Publication Date: 2014-02-18
• Subjects: stars: variables: δ Scuti, -- stars: variables: γ Doradus, -- pulsation driving mechanisms; Astronomy -- Congresses; Astronomy -- Periodicals; 520
• DOI: 10.1017/S1743921313014099
• Languages: English
• ISSNs: 1743-9213

Abstract

Abstract: We examine the light curves of over 2700 stars observed in long cadence by the Kepler spacecraft as part of the Guest Observer program. Most of these stars are faint ( Kepler magnitude > 14), and fall near or within the effective temperature and log g range of the γ Dor and δ Sct instability strips. We find that the pulsating stars are obvious from inspection of the light curves and power spectra, even for these faint stars. However, we find that a large number of stars are 'constant', i.e. show no frequencies in the 0.2 to 24 d −1 range above the 20 ppm level. We discuss the statistics for the constant stars, and some possible physical reasons for lack of pulsations. On the other hand, γ Dor and δ Sct candidates have been found in the Kepler data spread throughout and even outside of the instability regions of both types that were established from pre- Kepler ground-based observations. We revisit mechanisms to produce g- or p-mode pulsations in conditions when these modes are not expected to be unstable via the He-ionization κ effect (δ Sct) or convective blocking (γ Dor) pulsation driving mechanisms.