An Investigation of the Period Variations of the Eclipsing System V566-OPHIUCHI

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The period variations of the eclipsing variable V566 Oph were studied
with 112 moments of main minimum. The curve (O-C)-JD shows the system to
be composed of three stars rotating around the mass centre with the
period Π = 21 years and amsin i = 1.3×108km.

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