Ryu 200

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C3
N_50
r_50
AC 37 2.0
Summary

Ryu 200 is a poorly populated, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, well above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Bica et al. (2019) 269.342 -16.865
           
UCC 269.34 -16.872 0.106 -3.553 -6.08 26.956
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Ryu 200 UCC

Explore data in Colab

Search coordinates in Bayestar19

Cluster region map