Theoretical instability strips for δ Scuti and γ Doradus stars

By M. Dupret, A. Grigahcène, R. Garrido, M. Gabriel, R. Scuflaire. 2004

141 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/74a6c5f39e0bc9d5a546dae88ac5ad428c610464

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In Astronomy and Astrophysics

Citations in the corpus

TESTING SCALING RELATIONS FOR SOLAR-LIKE OSCILLATIONS FROM THE MAIN SEQUENCE TO RED GIANTS USING KEPLER DATA (2011, methodology): “Considerable work has been devoted to establishing this boundary both empirically using δ Scuti and γDoradus stars (see, e.g., Breger 1979; Pamyatnykh 2000) as well as theoretically (see, e.g., Houdek et al. 1999b; Houdek 2000; Xiong & Deng 2001; Dupret et al. 2004, 2005).”
The Kepler characterization of the variability among A- and F-type stars I. General overview (2011, background): “Our current understanding is that they pulsate in high-order gravity (g) modes (Kaye et al. 1999a), excitedby a flux modulation mechanism induced by the upper convective layer (Guzik et al. 2000; Dupret et al. 2004; Grigahcène 2005).”
Probing the properties of convective cores through g modes : high-order g modes in SPB and γ Doradus stars (2008, background): “The modulation of the radiative flux by convection at the base of the convective envelope was proposed as E-mail: j.montalban@ulg.ac.be the excitation mechanism for such stars (see e.g. Guzik et al. 2000; Dupret et al. 2004).”
MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): BINARIES, PULSATIONS, AND EXPLOSIONS (2015, result): “…the edges are somewhat cooler than results published in the literature; however, this is because we consider only fundamental and first-overtone modes, whereas the blue edge is typically set by higher overtones which are displaced toward hotter Teff (e.g., Dupret et al. 2004, their figure 1).”