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The Astrophysical Behavior of Open Clusters along the Milky Way Galaxy

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arxiv 1403.0621 v2 pith:CU25MLI2 submitted 2014-03-03 astro-ph.GA

A. L. Tadross This is my paper · ORCID
classification astro-ph.GA
keywords clustersastrophysicalopenalongbeenbehaviorgalaxymilky
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The main aim of this paper is to study the astrophysical behavior of open clusters' properties along the Milky Way Galaxy. Near-IR JHK (2MASS) photometry has been used for getting a homogeneous Catalog of 263 open clusters' parameters, which are studied for the first time by the author through the last five years. The correlations between the astrophysical parameters of these clusters have been achieved in morphological way and compared with the most recent works.

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Cited by 1 Pith paper

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

  1. Kings of the Milky Way: A Homogeneous Gaia DR3 Analysis of King Open Clusters and the Galactic Disc Metallicity Gradient

    astro-ph.GA 2026-08 conditional novelty 4.0 of 10

    A homogeneous Gaia DR3 re-analysis of all 27 King open clusters gives consistent parameters and a metallicity gradient of about -0.06 dex/kpc, but the King-only slope is not statistically significant as printed.

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