Constraints on stellar evolution from white dwarf asteroseismology

Research output: Contribution to journalArticle

Abstract

High mass and low mass stars follow a similar evolution until the inert core phase that follows the end of the core helium burning stage. In particular, one common phase of stellar evolution is the alpha capture reaction that turns carbon into oxygen in the core. We can obtain constraints on this reaction rate by studying the remnants of low mass stars, as this is the ultimate reaction that occurs in their core. We also present results that allow us to test the time dependent calculations of diffusion in dense interiors.

Original languageEnglish (US)
Pages (from-to)211-212
Number of pages2
JournalProceedings of the International Astronomical Union
Volume9
DOIs
StatePublished - Jan 1 2014

All Science Journal Classification (ASJC) codes

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Constraints on stellar evolution from white dwarf asteroseismology'. Together they form a unique fingerprint.

  • Cite this