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Table · dataset · 2025

Metallicities of old open clusters

Listed in IVOA Registry (Virtual Observatory)

We determined precise and homogeneous metallicities for old open clusters (>=500Myr) from all-sky catalogues of stellar parameters leveraging Gaia spectrophotometry.

Description

Our purpose was to revisit the metallicity distribution of the oldest open clusters as a function of their Galactic position and age with improved statistics. Several catalogues of stellar parameters have been cross-matched to the most recent census of open clusters and their members.

Median metallicities per cluster and per catalogue were evaluated by comparison to high-resolution spectroscopy. Our sample includes 1113 open clusters. A typical precision of 0.05dex is achieved for a subsample of nearly 600 clusters when only their bright red giants are considered.

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Metal-rich and metal-poor clusters never studied before are presented, as well as remnants of dissolving clusters. Galactic maps show a smooth decrease of metallicity from inside to outside the disc. We measured the radial and vertical gradients, their evolution with time and the age-metallicity relation in bins of Galactocentric distance.

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Provenance · 1 source records, 8 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/699/a24615 d agoJSON v1
FieldAssertionExtractorEvidence
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