Ryu 210

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C3
N_50
r_50
DD 20 1.8
Summary

Ryu 210 is a sparse, very dense object of very low C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.

This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Bica et al. (2019) 274.325 -16.933
           
UCC 274.312 -16.911 0.56 -0.784 -2.229 13.88
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Ryu 210 UCC

Explore data in Colab

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
VVVX CL093 32.0 274.38 -16.97 0.61 -1.54 -3.1 4.2 0.42
VVVX CL095 16.0 274.4 -16.93 0.52 -0.27 -2.16 -11.4 0.05
VVVX CL092 12.0 274.26 -17.08 0.56 -1.18 -2.63 0.1
VVVX CL087 4.0 274.07 -16.87 0.44 -1.13 -2.19 0.07