The field high-amplitude SX Phoenicis variable BL Camelopardalis: results from a multisite photometric campaign
Makaleler > Tam Makale · 2007
Yazarlar: E. Rodríguez, S. Fauvaud, J. A. Farrell, A.-Y. Zhou, J.-P. Sareyan, M. J. López-González, M.-A. Dupret, A. Grigahcéne, J. de Ridder, G. Klingenberg, M. Wolf, P. Van Cauteren, P. Lampens, D. Martínez, V. M. Casanova, F. J. Aceituno, M. Helvaci, E. G. Hintz, L. Král, F. Fumagalli, J. H. Simonetti, B. H. Granslo, L. Kotková, G. Santacana, J. Michelet, M. Fauvaud, J.-M. Vugnon, H. Sadsaoud, S. Aliouane, Z. C. Grigahcéne, S. Martín-Ruíz, P. J. Amado, J. C. Suárez, A. Moya, H. Kučáková, R. Kocián, K. Truparová, A. Avdibegović, M. Blažek, J. Kliner, P. Zasche, M. Vilásek, S. Bartošíková, B. Yasarsoy, C. Ulusoy, K. A. Graham, M. P. Nicholson, O. Trondal, C. Yesilyaprak, D. Coker
Astronomy & Astrophysics, Uluslararası, Wos, 2007, cilt 471, ss 255-264
DOI: 10.1051/0004-6361:20077514
Özet
Context.BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very complex frequency spectrum is detected, with a number of independent nonradial modes excited, unusual among the high-amplitude pulsators in the Lower Classical Instability Strip.