A new correction of stellar oscillation frequencies for near-surface effects

W. H. Ball, Laurent Gizon

Research output: Contribution to journalArticle

Abstract

Context. Space-based observations of solar-like oscillations present an opportunity to constrain stellar models using individual mode frequencies. However, current stellar models are inaccurate near the surface, which introduces a systematic difference that must be corrected.

Original languageEnglish (US)
Article numberA123
JournalAstronomy and Astrophysics
Volume568
DOIs
StatePublished - Aug 1 2014

Fingerprint

stellar oscillations
stellar models
oscillation
solar oscillations
effect

Keywords

  • Asteroseismology
  • Stars: individual: HD 52265
  • Stars: oscillations

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

A new correction of stellar oscillation frequencies for near-surface effects. / Ball, W. H.; Gizon, Laurent.

In: Astronomy and Astrophysics, Vol. 568, A123, 01.08.2014.

Research output: Contribution to journalArticle

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