Ryu 596

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.86 0.25 0.0 1.0
C3
N_50
r_50
CC 20 2.9
Summary

Ryu 596 is a sparse, dense object of low C3 quality. It is located at a moderate 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 object shares a small percentage of members with 3 later reported entries.

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) 270.221 -24.214 – – – –
           
UCC 270.219 -24.225 0.392 0.056 -1.418 25.136
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Ryu 596 UCC

Explore data in Colab

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 80 16.0 270.25 -24.33 0.35 0.12 -1.47 17.57 0.22
CWNU 4102 4.0 270.06 -24.29 0.47 0.09 -1.15 37.84 0.07
HSC 79 4.0 270.06 -24.29 0.48 0.09 -1.18 92.36 0.34