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

Astrophysics 2008-11-26 v1
Authors: A. Majewska-Swierzbinowicz , A. Pigulski , R. Szabo , Z. Csubry
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Abstract

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).

Cite

@article{arxiv.0711.1627,
  title  = {Pulsating B-type stars in the young open cluster h Persei (NGC 869)},
  author = {A. Majewska-Swierzbinowicz and A. Pigulski and R. Szabo and Z. Csubry},
  journal= {arXiv preprint arXiv:0711.1627},
  year   = {2008}
}

Comments

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

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