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The Fourier Decomposition of the Light Curves of High Amplitude δ Set Stars

Published online by Cambridge University Press:  12 April 2016

Ennio Poretti
Ennio Poretti*
Affiliation:
Osservatorio Astronomico di Brera, Via E. Bianchi 46, 1–23807 Merate, Italy

Abstract

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A significant improvement of the relationships between observed and physical properties of high amplitude δ Scuti stars (HADS), SX Phe stars, and RRc stars can be obtained by the systematic application of Fourier decomposition to their light curves.

Type
Part 1. Large Scale Surveys: Present and Future
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 83 - 84
Copyright
Copyright © Astronomical Society of the Pacific 2000

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