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Recovering the Pulsation Velocity Distribution on Stellar Surface
Published online by Cambridge University Press: 08 February 2017
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The analytical expression between the line profile and its corresponding pulsation velocity field is derived by the assumption of Doppler Imaging (DI). Based on this approach, numerical experiments of the recovery of the one dimensional nonradial pulsation velocity distribution from the residual line profiles are presented.
- Type
- VI. Asteroseismology II
- Information
- Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 383 - 384
- Copyright
- Copyright © Kluwer 1998
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