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

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dc.creatorMajewska-Swierzbinowicz, A.
dc.creatorPigulski, A.
dc.creatorSzabo, R.
dc.creatorCsubry, Z.
dc.date2007-11-10
dc.date.accessioned2026-07-07T11:54:06Z
dc.date.available2026-07-07T11:54:06Z
dc.descriptionWe 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).
dc.description5 pages, 5 figures, Proc. HELAS-II conference, Goettingen, 20-24 August 2007
dc.identifierhttps://arxiv.org/abs/0711.1627
dc.identifierhttp://arxiv.org/abs/0711.1627
dc.identifierJ.Phys.Conf.Ser.118:012068,2008
dc.identifierdoi:10.1088/1742-6596/118/1/012068
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/204777
dc.subjectAstrophysics
dc.titlePulsating B-type stars in the young open cluster h Persei (NGC 869)
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