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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.

Information

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

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