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Conference object . 2022
License: CC BY
Data sources: Datacite
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Other literature type . 2022
License: CC BY
Data sources: ZENODO
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Conference object . 2022
License: CC BY
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The solar neighbourhood age-metallicity relation from Gaia white dwarf-main sequence binaries

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type 27 Jun 2022Publisher:Zenodo
Authors: Rebassa-Mansergas, Alberto; Maldonado, Jesus; Knowles, Adam Thomas; Raddi, Roberto; Torres, Santi;

doi: 10.5281/zenodo.6761375 , 10.5281/zenodo.6761374

The solar neighbourhood age-metallicity relation from Gaia white dwarf-main sequence binaries

Abstract

The age-metallicity relation is a fundamental observational tool for constraining the chemical evolution of the Galactic disc in time. In this work we analyse the observational properties of this relation using binary stars that evolved avoiding mass transfer episodes consisting of a main sequence star - from which we can derive the metallicities - and a white dwarf - from which we can derive the total ages of the systems. Our sample consists of 189 WD+MS common proper motion pairs (CPMPs) identified within Gaia.

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This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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