CWNU 3476

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.33 0.13 0.75 0.0 1.0
C3
N_50
r_50
AB 33 5.4
Summary

CWNU 3476 is a poorly populated, very loose object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.

This object shares a very small 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) 121.704 -33.382 0.227 -2.389 2.632 –
           
UCC 121.721 -33.394 0.223 -2.389 2.637 64.312
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 3476 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.35, m-M=12.8, logA=7.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 5150 3.0 121.5 -33.05 0.21 -2.41 2.68 49.45 0.05