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 Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We explore the evolution of hydrogen-rich and hydrogen-deficient white dwarfstars with masses between 1.012 and 1.307 Msun, and initial metallicity ofZ=0.02. These sequences are the result of main sequence stars with massesbetween 8.8 and 11.8 Msun. The simulations were performed with MESA, startingat the zero-age main sequence, through thermally pulsing and mass-loss phases,ending at the white dwarfs cooling sequence. We present reliable chemicalprofiles for the whole mass range considered, covering the different expectedcentral compositions, i.e. C/O, O/Ne and Ne/O/Mg, and its dependence with thestellar mass. In addition, we present detailed chemical profiles of hybridC/O-O/Ne core white dwarfs, found in the mass range between 1.024 and 1.15Msun. We present the initial-to-final mass relation, mass-radius relation, andcooling times considering the effects of atmosphere and core composition.

New full evolutionary sequences of H and He atmosphere massive white dwarf stars using MESA