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g Modes in γ Doradus Stars: a Theoretician’s Quest for Instability

Published online by Cambridge University Press:  12 April 2016

W. Löffler
W. Löffler*
Affiliation:
Astronomical Institute, Graduate School of Science, Tohoku University, Sendai, Japan

Abstract

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We present a new implementation of the Riccati method for the linear stability analysis of weakly non-adiabatic g-mode pulsations in γ Doradus stars.

Type
Part 4. The Interaction between Convection and Pulsation
Information
International Astronomical Union Colloquium , Volume 185: Radial and Nonradial Pulsations as Probes of Stellar Physics , 2002 , pp. 508 - 509
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Gautschy, A., Glatzel, W. 1990, MNRAS, 245, 154 Google Scholar
Gautschy, A. 1996, private communicationGoogle Scholar
Löffler, W. 1999, PhD Thesis, Universitt Basel Google Scholar
Löffler, W. 2000, in ASP Conf. Ser., Vol. 203, The impact of Large-Scale Surveys on Pulsating Star Research, eds. Szabados, L. & Kurtz, D., (San Francisco: ASP), 447 Google Scholar
Muller, D.E. 1956, MTAC, 10, 208 Google Scholar
Pamyatnykh, A.A. 2000, in ASP Conf. Ser., Vol. 210, Delta Scuti and Related Stars, eds. Breger, M. & Montgomery, M., (San Francisco: ASP), 215 Google Scholar