The field high-amplitude SX Phoenicis variable BL Camelopardalis: results from a multisite photometric campaign
ASTRONOMY & ASTROPHYSICS, cilt.471, sa.1, ss.255-264, 2007 (SCI-Expanded, Scopus)
- Yayın Türü: Makale / Tam Makale
- Cilt numarası: 471 Sayı: 1
- Basım Tarihi: 2007
- Doi Numarası: 10.1051/0004-6361:20077514
- Dergi Adı: ASTRONOMY & ASTROPHYSICS
- Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
- Sayfa Sayıları: ss.255-264
- Anahtar Kelimeler: stars : variables : delta Sct, stars : individual : BL Camelopardalis, stars : oscillations, techniques : photometric, DELTA-SCUTI STARS, SCT STARS, PULSATION, ASTEROSEISMOLOGY, FREQUENCIES
- 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.