CWNU 3876

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.42 0.05 0.75 0.0 1.0
C3
N_50
r_50
AB 42 3.3
Summary

CWNU 3876 is a poorly populated, very loose object of high C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It was recently reported in the literature.

This object shares a significant percentage of members with a later reported entry.

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
He et al. (2023) 121.793 -41.303 0.069 -1.351 2.184 112.74
           
UCC 121.78 -41.306 0.072 -1.363 2.194 126.61
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 3876 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.6, m-M=15.2, logA=6.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2065 59.5 121.79 -41.31 0.07 -1.36 2.18 126.61 0.0