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Origin of the system of globular clusters in the Milky Way -- Gaia eDR3 edition

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arxiv 2503.14657 v1 pith:CD5YS6XS submitted 2025-03-18 astro-ph.GA

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keywords edr3gaiamassariassociationsavailableclustersdataedition
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In this research note I update the associations between globular clusters and their putative galaxy progenitors determined in Massari et al. (2019), based on the kinematic measurements from the Gaia early data release 3 (eDR3, Gaia Collaboration et al. 2021). The table with the associations is available at https://www.oas.inaf.it/en/research/m2-en/carma-en/, and will be kept up-to-date whenever improved data become available. The same table will also provide updated age estimates from the CARMA project (see Massari et al. 2023). Please cite this Note alongside Massari, Koppelman & Helmi 2019, eDR3 edition.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Isochrone fitting of Galactic globular clusters - IX. Tip of the red-giant branch for 27 clusters and constraints on new particle physics

    hep-ph 2026-08 conditional novelty 6.0 of 10

    No anomalous energy loss is seen in the red-giant tips of 27 globular clusters, yielding g_ae < 3.8e-14 at 95% confidence, the strongest bound for axion-electron coupling below about 1 keV.

  2. Constructing a Pristine View of Extended Globular Cluster Structure

    astro-ph.GA 2025-07 conditional novelty 5.0 of 10

    Extended tidal structure is identified around 22 Milky Way globular clusters using Pristine photometric metallicities and Gaia astrometry, including six new tentative detections.

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