CWNU 3844

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.33 0.24 0.12 0.0 0.97
C3
N_50
r_50
DC 33 3.4
Summary

CWNU 3844 is a poorly populated, very loose object of very low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.97) 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
He et al. (2023) 12.821 64.633 0.186 -1.769 -0.222 –
           
UCC 12.802 64.638 0.189 -1.785 -0.212 -72.749
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3844 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.7, m-M=14.35, logA=6.5

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2897 3.0 13.22 64.43 0.24 -2.0 -0.32 – 0.03