English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We present a large bank of chemical profiles and pulsation periods suited forasteroseismological studies of ZZ Ceti (or DAV) variable stars. Our backgroundequilibrium DA white dwarf models are the result of fully evolutionarycomputations that take into account the complete history of the progenitorstars from the ZAMS. The models are characterized by self-consistent chemicalstructures from the centre to the surface, and cover a wide range of stellarmasses, effective temperatures, and H envelope thicknesses. We present dipoleand quadrupole pulsation $g$-mode periods comfortably covering the interval ofperiods observed in ZZ Ceti stars. Complete tabulations of chemical profilesand pulsation periods to be used in asteroseismological period fits, as well asother quantities of interest, can be freely downloaded from our website(\url{http://www.fcaglp.unlp.edu.ar/evolgroup}

A public database for white dwarf asteroseismology with fully evolutionary models: I. Chemical profiles and pulsation periods of ZZ Ceti (DAV) stars