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astro-ph2002★ 80 cited
A photometric mode identification method, including an improved non-adiabatic treatment of the atmosphere
M. -A. Dupret, J. De Ridder, P. De Cat +4
We present an improved version of the method of photometric mode identification of Heynderickx et al. (1994). Our new version is based on the inclusion of precise non-adiabatic eig…
astro-ph2002
Searching for Line Profile Variability in HgMn Stars
S. Turcotte, C. Aerts, P. Knoglinger
Spectra of four non-magnetic chemically peculiar late B type stars (HgMn) stars are analysed to detect periodic spectral line variations (LPVs). A procedure developed to study LPVs…