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 Tools annual

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 monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

Mass loss is a crucial component in stellar evolution models, since itlargely determines the rate of evolution at the later stages of a star's life.The dust-driven outflows from AGB stars are particularly important in thisregard. Including AGB dust formation in a stellar evolution model does alsorequire a model of these outflows. Since AGB stars exhibit large-amplitudepulsation, a model based on time-dependent radiation hydrodynamics (RHD) isneeded in order to capture all the important physical aspects of dustformation. However, this cannot be afforded in a stellar evolution model. Here,a mean-flow model is presented, which include corrections to the steady-statemodel currently being used in AGB evolution models with dust formation.

Improved implementation of dust-driven winds and dust formation in models of AGB evolution: Effects of pulsation and gas-pressure forcing