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Tuning Pulsation Modes with Stellar Interferometry
Published online by Cambridge University Press: 12 April 2016
Abstract
Stellar interferometry represents a qualitative jump toward stellar surface imaging. We propose a method that tunes and filters out high degree non-radial pulsation (NRP) modes from the Fourier plane associated to the stellar brightness distribution. The proposed method can be applied to continuum flux, slow stellar rotation and high degree multi mode NRP stars.
- Type
- Part 1.5. General Aspects
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2002
Footnotes
Present address: Astronomical Observatory Beograd, Beograd, Yugoslavia