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Eigenfunctions of Axisymmetric p-modes in The Presence of A Dipole Magnetic Field: Observational Consequences
Published online by Cambridge University Press: 12 April 2016
Abstract
We calculate the effects of a 3.2-kG dipolar magnetic field on the eigenfunctions of high-order p-mode pulsations and discuss the consequences for pulsation amplitude modulation with rotation phase and for line profile variations.
- Type
- Part 8. New theoretical developments in stellar pulsation and variability
- Information
- International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 478 - 482
- Copyright
- Copyright © Astronomical Society of the Pacific 2004