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

Star clusters are fundamental building blocks of galaxies. Their formation isrelated to the density and pressure in progenitor molecular clouds and theirenvironmental conditions. To understand better the dynamical processes drivingstar formation and chemical evolution, we compare ages, metallicities, andalpha-element abundance ratios of globular clusters in nearby dwarf galaxies ofdifferent luminosities and morphological types, and situated in differentenvironments. The data are based on our 6m telescope medium-resolutionspectroscopic observations. We find that a mean metallicity of GCs in a galaxyat a given age is higher for early-type dwarfs, than for late-type dwarfirregulars and spirals.

Looking for a link between Gas Content of Dwarf Galaxies and Properties of their Globular Cluster systems