Atıf İçin Kopyala
Fauvaud S., Sareyan J. -., Ribas I., Rodriguez E., Lampens P., Klingenberg G., ...Daha Fazla
ASTRONOMY & ASTROPHYSICS, cilt.515, 2010 (SCI-Expanded)
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Yayın Türü:
Makale / Tam Makale
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Cilt numarası:
515
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Basım Tarihi:
2010
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Doi Numarası:
10.1051/0004-6361/201014243
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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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Anahtar Kelimeler:
stars: variables: delta Scuti, stars: individual: BL Camelopardalis, stars: oscillations, binaries: general, techniques: photometric, LONG-TERM VARIABILITY, DELTA-SCUTI STARS, STELLAR EVOLUTION, PHOENICIS STARS, DWARF CEPHEIDS, PERIOD CHANGES, CAMELOPARDALIS, STRAGGLERS, PLANETS, TRIPLE
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Atatürk Üniversitesi Adresli:
Evet
Özet
Context. Short-period high-amplitude pulsating stars of Population I (delta Sct stars) and II (SX Phe variables) exist in the lower part of the classical (Cepheid) instability strip. Most of them have very simple pulsational behaviours, only one or two radial modes being excited. Nevertheless, BL Cam is a unique object among them, being an extreme metal-deficient field high-amplitude SX Phe variable with a large number of frequencies. Based on a frequency analysis, a pulsational interpretation was previously given.