Preliminary analysis of photometric variations of central star of planetary nebula Sh 2-71

Astronomy and Astrophysics – Astrophysics

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4 pages, 3 figures, Proceedings of the conference: Zdenek Kopal's Binary Stars Legacy, March 31 - April 3, 2004, Litomysl, Cze

Scientific paper

10.1007/s10509-005-4884-2

We confirmed the presence of regular UBVRIc light variations of the object in
the centre of planetary nebula Sh 2-71, the improved period of them being P
=(68.132+/-0.005) days. The shapes and amplitudes of light curves in particular
colours are briefly discussed.

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