CWNU 2887

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.34 0.75 0.0 1.0
C3
N_50
r_50
BA 23 4.7
Summary

CWNU 2887 is a sparse, loose object of high C3 quality. It is located at a moderate distance from the Sun, 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) 264.381 -34.924 0.369 0.414 -1.97 10.96
           
UCC 264.379 -34.92 0.371 0.409 -1.988 10.964
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2887 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.15, m-M=11.9, logAge=8.8

Search coordinates in Bayestar19

Cluster region map