Atıf İçin Kopyala
Rodriguez E., Fauvaud S., Farrell J. A., Zhou A., Sareyan J., Lopez-Gonzalez M. J., ...Daha Fazla
ASTRONOMY & ASTROPHYSICS, cilt.471, sa.1, ss.255-264, 2007 (SCI-Expanded)
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Yayın Türü:
Makale / Tam Makale
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Cilt numarası:
471
Sayı:
1
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Basım Tarihi:
2007
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Doi Numarası:
10.1051/0004-6361:20077514
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Dergi Adı:
ASTRONOMY & ASTROPHYSICS
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Derginin Tarandığı İndeksler:
Science Citation Index Expanded (SCI-EXPANDED), Scopus
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Sayfa Sayıları:
ss.255-264
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Anahtar Kelimeler:
stars : variables : delta Sct, stars : individual : BL Camelopardalis, stars : oscillations, techniques : photometric, DELTA-SCUTI STARS, SCT STARS, PULSATION, ASTEROSEISMOLOGY, FREQUENCIES
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Akdeniz Üniversitesi Adresli:
Hayır
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.