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Limits for the application of spectroscopic mode ID methods

  • W. Zima (a1), K. Kolenberg (a1) (a2), M. Briquet (a2) and M. Breger (a1)

Abstract

Spectroscopic mode identification techiques, which monitor intensity variations across an absorption line, provide the possibility of determining the quantum numbers l and m, the inclination and the intrinsic pulsation amplitude of a star. Of course, the uncertainties of the mode identification are dependent on the quality of the observations and the identification method applied. We have focused on the Pixel-by-pixel method/Direct line profile fitting (Mantegazza 2000) and the Moment method (Balona 1987, Briquet & Aerts 2003) for pinpointing mode parameters and tested the impact of various observational effects and stellar properties on the identification.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

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Limits for the application of spectroscopic mode ID methods

  • W. Zima (a1), K. Kolenberg (a1) (a2), M. Briquet (a2) and M. Breger (a1)

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