Astron. Astrophys. Suppl. Ser.
Volume 136, Number 2, April II 1999
|Page(s)||285 - 292|
|Published online||15 April 1999|
Pulsation of the δ Scuti star VZ Cancri
Laboratoire d'Astrophysique de Toulouse, Observatoire Midi-Pyrénées, 14 avenue Édouard Belin, F-31400 Toulouse, France
2 Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China
Send offprint request to: J.-N. Fu
Accepted: 5 January 1999
After the "” technique is used to study the pulsation of the δ Scuti star VZ Cnc with the times of maximum light listed in the literature and a newly-determined time based on new photometry for this star, some high-quality photometry light curves in the literature are analysed by the Fourier decomposition, showing that there are more than 2 frequencies in the pulsation of this star, which might be one possible explanation of the existence of the large scatter in the "” diagram.
Key words: δ Sct variable / VZ Cnc / oscillations
© European Southern Observatory (ESO), 1999