The connection between period spectra and constraints in white dwarf asteroseismology

Research output: Chapter in Book/Report/Conference proceedingConference contribution

3 Scopus citations

Abstract

White dwarfs are the end product of evolution for around 98% of the stars in our Galaxy. Buried in their interiors are the records of physical processes that take place during earlier stages in the life of the star. In recent years, a well-established theory of non-radial oscillations, improved white dwarf models, year of expertise built up in the field of white dwarf asteroseismic fitting, and computing power have culminated in the asteroseismology finally delivering what it promised: a detailed map of the interior structure of white dwarfs. As always in science, new results raise new questions. We perform a number of numerical experiments to better understand the connection between a given set of periods varying in the number of periods and in the set of radial overtones and the quality of the constraints on interior structure one obtains from fitting these periods.

Original languageEnglish (US)
Title of host publicationWide-Field Variability Surveys
Subtitle of host publicationA 21st Century Perspective - 22nd Los Alamos Stellar Pulsation - Conference Series Meeting
EditorsWolfgang Gieren, Marcio Catelan, Wolfgang Gieren, Marcio Catelan
PublisherEDP Sciences
ISBN (Electronic)9782759890248
DOIs
StatePublished - Sep 8 2017
Event22nd Los Alamos Stellar Pulsation Conference Series Meeting 2016 - San Pedro de Atacama, Chile
Duration: Nov 28 2016Dec 2 2016

Publication series

NameEPJ Web of Conferences
Volume152
ISSN (Print)2101-6275
ISSN (Electronic)2100-014X

Other

Other22nd Los Alamos Stellar Pulsation Conference Series Meeting 2016
Country/TerritoryChile
CitySan Pedro de Atacama
Period11/28/1612/2/16

All Science Journal Classification (ASJC) codes

  • General Physics and Astronomy

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