Seven-period asteroseismic fit of the Kepler DBV

Agnès Bischoff-Kim, Roy H. Østensen, J. J. Hermes, Judith L. Provencal

Research output: Contribution to journalArticle

20 Scopus citations

Abstract

We present a new, better-constrained asteroseismic analysis of the helium-atmosphere (DB) white dwarf discovered in the field of view of the original Kepler mission. Observations obtained over the course of 2 yr yield at least seven independent modes, two more than were found in the discovery paper for the object. With several triplets and doublets, we are able to fix the ℓ and m identification of several modes before performing the fitting, greatly reducing the number of assumptions we must make about mode identification. We find a very thin helium layer for this relatively hot DB, which adds evidence to the hypothesis that helium diffuses outward during DB cooling. At least a few of the modes appear to be stable on evolutionary timescales and could allow us to obtain a measurement of the rate of cooling with monitoring of the star over the course of the next few years with ground-based follow-up.

Original languageEnglish (US)
Article number39
JournalAstrophysical Journal
Volume794
Issue number1
DOIs
StatePublished - Oct 10 2014

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Seven-period asteroseismic fit of the Kepler DBV'. Together they form a unique fingerprint.

  • Cite this