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An Improved Method of Photometric Mode Identification: Applications to Slowly Pulsating B, ß Cephei, δ Scuti and γ Doradus Stars
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An Improved Method of Photometric Mode Identification: Applications to Slowly Pulsating B, ß Cephei, δ Scuti and γ Doradus Stars
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Dupret, M.-A.
et al
- published in Astrophysics and Space Science, 284, pp. 129-132 (2003) - ASTROimport-98
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