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 review the state of our chemical evolution models for spiral and low massgalaxies. We analyze the consequences of using different stellar yields, infallrate laws and star formation prescriptions in the time/redshift evolution ofthe radial distributions of abundances, and other quantities as star formationrate or gas densities, in the Milky Way Galaxy; In particular we will study theevolution of the Oxygen abundance radial gradient analyzing its relation withthe ratio SFR/infall. We also compare the results with our old chemicalevolution models, cosmological simulations and with the existing data, mainlywith the planetary nebulae abundances.

The evolution of the Oxygen abundance radial gradient in the Milky Way Galaxy disk