2003
Ref: ASTROimport-98

An Improved Method of Photometric Mode Identification: Applications to Slowly Pulsating B, ß Cephei, δ Scuti and γ Doradus Stars

Dupret, M.-A. ; Scuflaire, R. ; Noels, A. ; Thoul, A. ; Garrido, R. ; Moya, A. ; De Ridder, J. ; De Cat, P. ; Aerts, C.


published in Astrophysics and Space Science, 284, pp. 129-132 (2003)

Abstract: We 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.

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Royal Observatory of Belgium > Astronomy & Astrophysics
Science Articles > Peer Reviewed Articles



 Record created 2016-07-01, last modified 2016-07-01