HR4975 - a Possible Early-Type Contact System with Unequal Components

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

From 295 measurements in the Geneva seven-colour photometric system, it is found that the suspected variable star HR 4975 is in fact a close binary system. The colour variations and the very short period (0.64254 d) indicate a possible contact configuration. It is also argued that the two components are probably unequal in size and that the system is near to the ZAMS. Theoretical implications are briefly discussed.

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