CWWDL 14587

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.37 0.75 0.0 0.76
C3
N_50
r_50
AB 21 29.6
Summary

CWWDL 14587 is a sparse, loose object of high C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a 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=0.76) 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) 122.501 -49.83 2.58 -5.43 8.335 22.191
           
UCC 122.071 -49.849 2.565 -5.399 8.331 17.422
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 14587 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=6.04, Z=0.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 199 24.0 119.78 -49.16 2.47 -5.39 8.25 20.01 0.43