Bibcode
Li, Z.-P.; Michel, E.; Fox Machado, L.; Álvarez, M.; Chevreton, M.; Hernández, M. M.; Zhou, A. Y.; Barban, C.; Dolez, N.; Belmonte, J. A.; Fernandez, A.; Fremy, J.-R.; Pau, S.; Servan, B.; Pérez Hernández, F.; Jiang, S. Y.; Liu, Z. L.; Ringot, O.; Suárez, J. C.; Xu, Y.
Referencia bibliográfica
Astronomy and Astrophysics, v.420, p.283-287 (2004)
Fecha de publicación:
6
2004
Revista
Número de citas
12
Número de citas referidas
9
Descripción
New observations of V534 Tau were performed during the STEPHI IX
campaign in November 1998. An overall run of 285 h of data has been
collected from three sites over a period of 23 days. Period analysis
reveals a rich oscillation spectrum with nine frequencies above the 99%
confidence level. This oscillation spectrum spans a large range of
frequencies, from 179 to 525 μHz (15.52 to 45.36 cycles per day). A
preliminary comparison with models suggests that the observed modes
would lie in the range of modes from g1 or g2 to
p4 or p5, depending on the rotation rate
considered for V534 Tau.
Table
ef{tab1} is only available in electronic form at
http://www.edpsciences.org