Bibcode
Hernandez, M. M.; Michel, E.; Belmonte, J. A.; Jiang, S. Y.; Alvarez, M.; Chevreton, M.; Paparo, M.; Kjeldsen, H.; Bauduin, D.; Fromage, J.; Goupil, M. J.; Li, Z. P.; Liu, Y. Y.; Mangeney, A.; Massacrier, G.; Ringot, O.; Cortes, T. Roca; Servan, B.; Vidal, I.
Bibliographical reference
Astronomy and Astrophysics, v.337, p.198-206 (1998)
Advertised on:
9
1998
Journal
Citations
14
Refereed citations
11
Description
New observations of BS and BT Cnc were performed during the STEPHI VII
campaign in 1996 February. An overall run of 115 hours of data was
collected. Different methods have been used to analyse the time series,
bringing the detection of 2 frequencies for BT Cnc and 3 frequencies for
BS Cnc above the 99% confidence level. A comparison with the literature
reveals that the dominant mode of BT Cnc ( ~ 9.8 c/d) has kept excited
over tens of years, while the secondary modes have not been the same all
the time. However, during the very last years the two frequencies
detected by us have been the only ones noticeably excited in the
spectrum.