CWWDL 10590

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.02 0.25 0.0 1.0
C3
N_50
r_50
CC 13 11.7
Summary

CWWDL 10590 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.

This object shares a very small percentage of members with 2 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
Chi et al. (2023) 30.61 61.465 0.347 -0.002 -0.488 -72.293
           
UCC 30.555 61.476 0.291 0.032 -0.483 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 10590 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=7.82, Z=0.44

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3598 4.0 30.63 61.46 0.29 0.36 -0.44 – 0.01
HSC 1066 4.0 30.62 61.46 0.29 0.36 -0.44 – 0.48