Ryu 336

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.42 0.25 0.0 0.96
C3
N_50
r_50
CC 21 2.0
Summary

Ryu 336 is a sparse, loose object of low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.

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

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) 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) 247.9 -44.176 – – – –
           
UCC 247.869 -44.173 0.184 -5.165 -6.353 -49.999
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Ryu 336 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 CL041 4.0 247.88 -44.17 0.05 -4.51 -5.6 -75.4 0.15