PPMXL and Gaia Morphological Analysis of Melotte 22 (Pleaides) and 25 (Hyades)
W. H. Elsanhoury, M. I. Nouh

TL;DR
This study conducts a detailed morphological, photometric, and kinematic analysis of the open clusters Melotte 22 (Pleiades) and Melotte 25 (Hyades) using Gaia DR2 and PPMXL data, estimating their physical parameters and dynamical states.
Contribution
It provides new estimates of cluster parameters, masses, and kinematic properties, and assesses their dynamical relaxation status using Gaia and PPMXL data.
Findings
Clusters are dynamically relaxed based on relaxation times.
Estimated cluster masses are approximately 662 and 514 solar masses.
Derived kinematic parameters agree with existing literature.
Abstract
In this article, we present a morphological study of the well-known extended sized open clusters in the sky, Melotte 22 (Pleiades) and Melotte 25 (Hyades) with J, H, and Ks regions due to Gaia DR2 and PPMXL catalogues. Based on proper motions of these clusters, we extract our candidates and hence constructing fitting isochrones with Solar metallicity Z = 0.019, log (age) = 8.2 +- 0.05 for Melotte 22, and metallicity Z = 0.024, log (age) = 8.9 +- 0.10 for Melotte 25. Some photometric parameters are estimated, e.g. cluster heliocentric distances are 135 +- 3.6 and 47.51 +- 2.15 pc respectively, luminosity and mass functions with mass-luminosity relation MLR of the second order polynomial, and we have estimated the masses of Melotte 22 and Melotte 25 as 662.476 +- 25.73 Msun and 513.819 +- 22.65 Msun. The relaxation times of these clusters are smaller than the estimated cluster ages, which…
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