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

We present a detailed abundance analysis of giant stars in NGC 1978, amassive, intermediate-age stellar cluster in the Large Magellanic Cloud,characterized by a high ellipticity and suspected to have a metallicity spread.We analyzed 11 giants, all cluster members, by using high resolution spectraacquired with the UVES/FLAMES spectrograph at the ESO-Very Large Telescope. Wefind an iron content of [Fe/H]=-0.38 dex with very low (0.07 dex) dispersion,and a mean heliocentric radial velocity Vr=293.1 (with an error of 0.9 km/s)and a velocity dispersion (3.1 km/s), thus excluding the presence of asignificant metallicity, as well as velocity, spread within the cluster.Comment: 14 pages, 4 figures, accepted for publication by Apj

On the Iron Content of NGC 1978 in the LMC: A Metal-rich, Chemically Homogeneous Cluster