CWNU 4251

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.13 0.62 0.0 1.0
C3
N_50
r_50
AC 19 1.5
Summary

CWNU 4251 is a sparse, very loose object of intermediate 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.

Warning: contains less than 25 stars with P>0.5 estimated.

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) 136.311 -54.977 0.084 -2.412 2.813 –
           
UCC 136.309 -54.976 0.081 -2.41 2.834 100.448
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4251 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.95, m-M=15.4, logA=8.7

Search coordinates in Bayestar19

Cluster region map