CWNU 3854

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.02 0.5 0.0 0.76
C3
N_50
r_50
BB 13 6.3
Summary

CWNU 3854 is a sparse, very loose object of intermediate C3 quality. It is located at a large 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=0.76) 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) 164.706 -60.983 0.171 -5.591 2.258 –
           
UCC 164.7 -60.983 0.167 -5.593 2.243 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3854 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.3, m-M=15.1, logA=6.5

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Majaess 133 24.0 164.66 -61.18 0.11 -5.52 2.29 32.4 0.72