Pulsating B-type stars in the young open cluster h Persei (NGC 869)

Astronomy and Astrophysics – Astrophysics

Scientific paper

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5 pages, 5 figures, Proc. HELAS-II conference, Goettingen, 20-24 August 2007

Scientific paper

10.1088/1742-6596/118/1/012068

We announce the discovery of six Beta Cephei stars and many other variable
stars in the young open cluster h Persei (NGC 869). The cluster seems to be
very rich in variable B-type stars, similarly to its twin, Chi Persei (NGC
884).

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