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Title:
Spatial wavelet analysis of line-profile variations
Authors:
Townsend, R. H. D.
Affiliation:
AA(Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT)
Publication:
Monthly Notices of the Royal Astronomical Society, Volume 310, Issue 3, pp. 851-862. (MNRAS Homepage)
Publication Date:
12/1999
Origin:
MNRAS
MNRAS Keywords:
LINE: PROFILES, METHODS: DATA ANALYSIS, STARS: EARLY-TYPE, STARS: OSCILLATIONS
DOI:
10.1046/j.1365-8711.1999.02996.x
Bibliographic Code:
1999MNRAS.310..851T

Abstract

The technique of wavelet analysis is discussed in the context of line-profile variations in rapidly rotating stars undergoing non-radial pulsation. This technique may be used to determine the harmonic degree l of the pulsation using isolated residual spectra; it is able to handle spectra with relatively low signal-to-noise ratio levels, and is well suited to extracting previously unobtainable information from low-quality, patchy data. A demonstration of the technique is presented using data generated from a spectral synthesis code.

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