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

W. H. Ball, L. 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

Keywords

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

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'A new correction of stellar oscillation frequencies for near-surface effects'. Together they form a unique fingerprint.

  • Cite this