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 develop an approach for fitting the results of modeling of wrigglingradial large scale iron pattern along the Galactic disk, derived over young(high massive) Cepheids, with the metallicity distribution, obtained using lowmass long living dwarf stars in the close solar vicinity. For this, at the stepof computing of the theoretical abundance distribution over low mass stars inthe solar vicinity we propose to redefine the initial mass function so as theresulting theoretical stellar distribution over masses would be close to thedistribution in the observed sample. By means of the above algorithm andsubsequent corrections of the theoretical metallicity distribution function,described in literature, we have achieved fairly well agreement of thetheoretical and observed metallicity distribution functions for low mass starsin the local solar vicinity.

Local metallicity distribution function derived from Galactic large-scale radial iron pattern modelling