Photometric multi-site campaign on massive B stars in the open cluster chi Persei (NGC 884)

Bildiriler > Tam Metin Bildiri · 2007

Yazarlar: S. Saesen, A. Pigulski, F. Carrier, J. De Ridder, C. Aerts, G. Handler, A. Narwid, J. N. Fu, C. Zhang, X. J. Jiang, G. Kopacki, J. Vanautgaerden, M. Steslicki, B. Acke, E. Poretti, K. Uytterhoeven, W. De Meester, M. D. Reed, Z. Kolaczkowski, G. Michalska, E. Schmidt, R. Ostensen, C. Gielen, K. Yakut, A. Leitner, Belinda KALOMENİ YAKUT, S. Prins, V. Van Helshoecht, W. Zima, R. Huygen, B. Vandenbussche, P. Lenz, D. Ladjal, E. Puga Antolin, T. Verhoelst, P. Niarchos, A. Liakos, D. Lorenz, S. Dehaes, M. Reyniers, G. Davignon, S-L Kim, D. H. Kim, Y-J Lee, C-U Lee, J-H Kwon, E. Broeders, H. Van Winckel, E. Vanhollebeke, G. Raskin, Y. Blom, J. R. Eggen, P. Beck, J. Puschnig, L. Schmitt, G. A. Gelven, B. Steiniger, R. Drummond

International Conference on Helioseismology, Asteroseismology and MHD Connections (HELAS II), Almanya, Uluslararası, Sözlü Sunum, Tam Metin Bildiri, 2007-2008, Wos, cilt 118, ss 012071-012071

DOI: 10.1088/1742-6596/118/1/012071

Özet

In 2005 a photometric observation campaign started on the open cluster χ Persei, involving 13 telescopes spread over the whole northern hemisphere. After two years we gathered almost 1200 hours of data. We present here preliminary results on the variability search, especially from the 60-cm telescope in Bialków (Poland), which show seven confirmed β Cephei stars, four candidate B-type pulsators and other interesting variable stars.

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