The field high-amplitude SX Phoenicis variable BL Camelopardalis: results from a multisite photometric campaign


Rodriguez E., Fauvaud S., Farrell J. A., Zhou A., Sareyan J., Lopez-Gonzalez M. J., ...More

ASTRONOMY & ASTROPHYSICS, vol.471, no.1, pp.255-264, 2007 (SCI-Expanded) identifier identifier

  • Publication Type: Article / Article
  • Volume: 471 Issue: 1
  • Publication Date: 2007
  • Doi Number: 10.1051/0004-6361:20077514
  • Journal Name: ASTRONOMY & ASTROPHYSICS
  • Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Page Numbers: pp.255-264
  • Keywords: stars : variables : delta Sct, stars : individual : BL Camelopardalis, stars : oscillations, techniques : photometric, DELTA-SCUTI STARS, SCT STARS, PULSATION, ASTEROSEISMOLOGY, FREQUENCIES
  • Akdeniz University Affiliated: No

Abstract

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.