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The Accurate Period of GX Aurigae

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Jiři Borovička

Stef‡nik Observatory, Petr’n 205, Prague 1, Czechoslovakia

Presented at the First European Meeting of the AAVSO Brussels, July 24-28, 1990

Abstract

Published times of minima and ten new visual timings of minima are used to derive new light elements for GX Aur, a Beta Lyrae type star.