CWNU 449

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.28 0.12 0.25 0.0 1.0
C3
N_50
r_50
CC 28 34.5
Summary

CWNU 449 is a poorly populated, very loose object of low C3 quality. It is located at a close distance from the Sun, near 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. (2022) 74.868 45.649 1.47 -1.29 -2.99 10.2
           
UCC 74.635 45.795 1.493 -1.293 -2.97 -7.8
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 449 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=0.6, m-M=9.2, logAge=7.9, Z=0.038

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 560 64.3 73.66 45.93 1.49 -1.29 -2.97 -7.69 0.04