CWWDL 1988

Click to load Aladin Lite
UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.26 0.17 0.38 0.0 0.77
C3
N_50
r_50
BC 26 6.9
Summary

CWWDL 1988 is a poorly populated, 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 is very likely a unique object, which shares a small percentage of members with at least one previously reported entry, and a small percentage with at least one entry reported in the same catalogue.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.77) 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) 6.807 62.946 0.359 -2.917 -0.83 -58.869
           
UCC 6.709 62.941 0.358 -2.958 -0.842 -115.411
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 1988 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=7.25, Z=0.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 410 23.1 6.98 62.95 0.35 -3.14 -1.02 -184.77 0.45
CWWDL 10495 11.5 7.34 62.97 0.33 -2.74 -0.77 -93.16 0.07