Ryu 151

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C3
N_50
r_50
DC 18 2.8
Summary

Ryu 151 is a sparse, very loose object of very low C3 quality. It is located at a very 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: contains less than 25 stars with P>0.5 estimated.

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) 261.178 -26.554
           
UCC 261.183 -26.569 0.066 -5.212 -7.608 148.201
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Ryu 151 UCC

Explore data in Colab

Search coordinates in Bayestar19

Cluster region map