CWWDL 4637

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.07 0.38 0.0 0.8
C3
N_50
r_50
BC 21 10.6
Summary

CWWDL 4637 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below 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=0.8) 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) 36.988 57.561 0.36 -0.321 -0.9 -31.417
           
UCC 37.053 57.675 0.392 -0.328 -0.906 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 4637 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=5.78, Z=0.44

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 191 20.0 37.49 58.06 0.41 -0.4 -0.95 -46.84 0.24