Photometric Modal Discrimination in Δ Scuti and Γ Doradus Stars

Abstract. The potential of photometric methods for the identification of l, the degree of spherical surface harmonic of a pulsating star, is investigated with special emphasis on Strömgren photometry applied to δ Scuti and γ Dor variables. Limitations of actual model atmospheres when fine precision is required for the calculations of partial derivatives and integrals, which depend on limb darkening coefficients, are discussed. Two methods are discussed to calculate the phase lags, the angle between maximum temperature and minimum radius, and R, a parameter which describes departure from adiabaticity of the atmospheres of these pulsating stars. These quantities appear to be very dependent on the convection as parametrized by the mixing length theory. When one of the methods is applied to the γ Dor stars gives phase lags close to 0◦, which are 90◦ − 180◦ out of phase from typical δ Scuti stars. Examples are given for some High Amplitude Delta Scuti Stars (HADS) where the method can be easily applied and gives results consistent to interpret them as radial (l=0) pulsating stars. Other low amplitude δ Scuti stars could be oscillating in a non-radial (l=1, 2) mode. Multi-band photometry is concluded to be a very powerful tool for mode identification of δ Scuti and γ Dor stars, specially with the more accurate photometry that will be achieved in the near future with the asteroseismological space missions now in progress.