000001941 001__ 1941
000001941 005__ 20160701171655.0
000001941 037__ $$aASTROimport-98
000001941 100__ $$aDupret, M.-A.
000001941 245__ $$aAn Improved Method of Photometric Mode Identification: Applications to Slowly Pulsating B, ß Cephei, δ Scuti and γ Doradus Stars
000001941 260__ $$c2003
000001941 520__ $$aWe present an improved version of the method of photometric mode identification based upon the inclusion of non-adiabatic eigenfunctions determined in the stellar atmosphere, according to the formalism recently proposed by Dupret et al. (2002). We apply our method to ß Cephei, Slowly Pulsating B, δ Scuti and γ Doradus stars. Besides identifying the degree l of the pulsating stars, our method is also a tool for improving the knowledge of stellar interiors and atmospheres, by imposing constraints on the metallicity for ß Cephei and SPBs, the characteristics of the superficial convection zone for δ Scuti and γ Doradus stars and the limb-darkening law. 
000001941 700__ $$a Scuflaire, R.
000001941 700__ $$a Noels, A.
000001941 700__ $$a Thoul, A.
000001941 700__ $$a Garrido, R.
000001941 700__ $$a Moya, A.
000001941 700__ $$a De Ridder, J.
000001941 700__ $$a De Cat, P.
000001941 700__ $$a Aerts, C.
000001941 773__ $$c129-132$$i1$$pAstrophysics and Space Science$$v284$$y2003
000001941 85642 $$ahttp://esoads.eso.org/abs/2003Ap%26SS.284..129D
000001941 905__ $$apublished in
000001941 980__ $$aREFERD