On the binary nature of the SX Phoenicis star CY Aqr

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Observations of a new time of maximum light of CY Aqr, an extensively-observed SX Phoenicis star, have been investigated in combination with the data presented in the literature for almost 7 decades. The O - C diagram reveals that the long-term period change of CY Aqr can be represented by a linear period change combined with the light-time effect in a highly-eccentric orbit with a period of half a century. The binary nature of CY Aqr is therefore discussed with emphasis on the light-time effect procedure.

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