Volume 420, Number 1, June II 2004
|Page(s)||283 - 287|
|Section||Stellar structure and evolution|
|Published online||14 May 2004|
9+ frequencies for V534 Tauri, a δ Scuti variable in the Pleiades*
Results of the STEPHI IX campaign
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, PR China
2 Observatoire de Paris, LESIA, UMR 8109, 92195 Meudon, France
3 Instituto de Astrofí sica de Canarias, 38200 La Laguna, Tenerife, Spain
4 Instituto de Astronomí a – UNAM, Ap.P. 877, Ensenada, BC, Mexico
5 National Solar Observatory, Tucson AZ 85719, USA
6 Observatoire Midi-Pyrénées, LAT, UMR 5572, 31400 Toulouse, France
7 Observatoire de Paris, GEPI, FRE 2459, 92195 Meudon, France
8 Departamento de Astrofísica, Universidad de La Laguna, Tenerife, Spain
Corresponding author: Z.-P. Li, email@example.com
Accepted: 8 March 2004
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.
Key words: galaxy: open clusters and associations: general / stars: variables: δ sct / stars: oscillations / stars: individuals: V534 Tau
© ESO, 2004
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.