Journal
ASTRONOMY & ASTROPHYSICS
Volume 382, Issue 2, Pages 556-562Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20011668
Keywords
stars : oscillations; stars : variables : delta Sct; stars : individual : HD 23156, HD 23194
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The results of the tenth multi-site campaign of the STEPHI network are reported. The delta Scuti stars V624 Tau (HD 23156) and HD 23194, belonging to the Pleiades cluster, were observed photometrically for 34 days on three continents during 1999 November-December. An overall run of 343 hours of data was collected. Seven frequencies for V624 Tau and two frequencies for HD 23194 have been found above a 99% confidence level. These results greatly improve those found in previous studies with much less data. A preliminary comparison of observed and theoretical frequencies suggests that both stars may oscillate with radial and non-radial p modes of radial orders typical among delta Scuti stars.
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