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Orbits of 152 Globular Clusters of the Milky Way Galaxy Constructed from the Gaia DR2 data

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arxiv 2008.13624 v3 pith:RY6DFZDY submitted 2020-08-28 astro-ph.GA

Orbits of 152 Globular Clusters of the Milky Way Galaxy Constructed from the Gaia DR2 data

classification astro-ph.GA
keywords clustersglobularorbitsdatagaiagalacticgalaxymilky
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We present orbits and their properties for 152 globular clusters of the Milky Way galaxy obtained using average Gaia DR2 proper motions and other astrometric data from the list of Vasiliev (2019). For orbit integrating we have used the axisymmetric model of the Galactic potential based on the Navarro-Frenk-White dark halo, and modified by Bajkova and Bobylev (2016) using circular velocities of Galactic objects in wide region of Galactocentric distances (up to 200 kpc) from Bhattacharjee et.al. (2014) catalog. Based on the analysis of the obtained orbits, we have modified the composition of the subsystems of globular clusters presented in Massari et. al. (2019).

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Cited by 1 Pith paper

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

  1. Neighbors, Not Kin: Kinematic evidence for tidal tails from NGC 7492 along the Sagittarius stream

    astro-ph.GA 2026-07 accept novelty 6.0

    GIRAFFE radial velocities and metallicities confirm NGC 7492 tidal tails extending ≥1.8 deg, kinematically and chemically distinct from the overlapping Sagittarius stream.