CWNU 1888

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.62 0.62 0.0 1.0
C3
N_50
r_50
AC 24 2.9
Summary

CWNU 1888 is a sparse, moderately dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, near 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) 11.625 63.23 0.31 -2.555 -0.433 –
           
UCC 11.619 63.238 0.303 -2.563 -0.42 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1888 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.55, m-M=12.5, logAge=6.9

Search coordinates in Bayestar19

Cluster region map