Long term photometric monitoring with the Mercator telescope
Makaleler > Tam Makale · 2006
Yazarlar: P. De Cat, M. Briquet, C. Aerts, K. Goossens, S. Saesen, J. Cuypers, Kadri YAKUT, R. Scuflaire, M. -A. Dupret, K. Uytterhoeven, H. Van Winckel, G. Raskin, G. Davignon, L. Le Guillou, R. Van Malderen, M. Reyniers, B. Acke, W. De Meester, J. Vanautgaerden, B. Vandenbussche, T. Verhoelst, C. Waelkens, P. Deroo, K. Reyniers, M. Ausseloos, E. Broeders, J. Daszynska-Daskiewicz, J. Debosscher, S. De Ruyter, K. Lefever, G. Decin, K. Kolenberg, A. Mazumdar, C. Van Kerckhoven, J. De Ridder, R. Drummond, C. Barban, E. Vanhollebeke, T. Maas, L. Decin
Astronomy & Astrophysics, SCI Expanded İndekslerine Giren Dergi, Uluslararası, Wos, 2006, cilt 463, ss 243-249
DOI: 10.1051/0004-6361:20066202
Özet
Aims. We selected a large sample of O-B stars that were considered as (candidate) slowly pulsating B, β Cep, and Maia stars after the analysis of their hipparcos data. We analysed our new seven passband geneva data collected for these stars during the first three years of scientific operations of the mercator telescope. We performed a frequency analysis for 28 targets with more than 50 high-quality measurements to improve their variability classification. For the pulsating stars, we tried both to identify the modes and to search for rotationally split modes.