A new period and period trend of IZ Persei

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Eclipsing Binary Stars, Periodic Variations, Tables (Data), Time Measurement

Scientific paper

A new period (P = 3d.687664) of the eclipsing binary system IZ Persei is given, based on 16 observed times of the minima. O-C diagrams of IZ Per have been presented for the first time, and the period variation have been estimated in different portions of the O-C diagram. The overall picture of IZ Per suggests that strong period changes are not present in the system; however a slow increase of period at a rate of 25syr-1 is apparent in IZ Per. The total period change (3×10-6d) till the last epoch is in agreement with the newly derived period of IZ Per.

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