Communications in Asteroseismology

By M. Breger, Daniel Klotz, P. Beck, C. Aerts, G. Handler, D. Kurtz, J. Matthews, E. Poretti. 2009

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Determining global parameters of the oscillations of solar-like stars (2009, unknown): “Thus, an independent determination of one of these two parameters (rotation or inclination angle) could help during the fitting procedure of the p-mode parameters to establish, for example, some a priori constraints (e.g. Benomar 2008; Benomar et al. 2009).”
White Dwarf Rotation as a Function of Mass and a Dichotomy of Mode Line Widths: Kepler Observations of 27 Pulsating DA White Dwarfs through K2 Campaign 8 (2017, background): “where Ck,l represents the effect of the Coriolis force on the pulsations, as formulated by Ledoux (1951). For high-k modes that approach the asymptotic, mode-independent limit for l = 1 modes, Ck,1 → 0.50. However, the low-k (especially k < 10) modes found in hot DAVs can suffer from strong mode-tra”