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An Attempt at Mode Identification for V480 Tau

Published online by Cambridge University Press:  12 April 2016

M.P. Di Mauro
Affiliation:
Theoretical Astrophysics Center, Aarhus, Denmark
J. Christensen-Dalsgaard
Affiliation:
Theoretical Astrophysics Center, Aarhus, Denmark
F. Pijpers
Affiliation:
Theoretical Astrophysics Center, Aarhus, Denmark
J. Hao
Affiliation:
Beijing Astronomical Observatory, Chin. Acad. of Sciences, P.R. China

Abstract

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Spectroscopic observations of the δ Scuti star V480 Tau, obtained during the MUSICOS 1996 campaign (Hao et al., 2001), detected a large number of modes. In order to assess the information available from such data, we compare the observed spectrum of frequencies with the theoretical predictions obtained for models computed by including the effect of fast rotation on global oscillations.

Type
Part 2.4. Delta Scuti Stars
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Abt, H.A., & Morrell, N.I. 1995, ApJS, 99, 135 CrossRefGoogle Scholar
Bahcall, J.N., & Pinsonneault, M.H. 1992, Rev. Mod. Phys., 64, 885 CrossRefGoogle Scholar
Christensen-Dalsgaard, J., Bedding, T.R., & Kjeldsen, H. 1995, ApJ, 443, L29 CrossRefGoogle Scholar
Christensen-Dalsgaard, J., & Thompson, M.J. 1999, A&A, 350, 852 Google Scholar
Eggleton, P.P., Faulkner, J., & Flannery, B.P. 1973, A&A, 23, 325 Google Scholar
Hao, J., Kennelly, E.J., Catala, C., et al. 2001, to be submitted to A&AGoogle Scholar
Iglesias, C.A., & Rogers, F.J. 1996, ApJ, 464, 943 CrossRefGoogle Scholar
Solano, E., & Fernley, J. 1997, A&AS, 122, 131 Google Scholar