CWNU 4190

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.1 0.38 0.0 0.96
C3
N_50
r_50
BC 19 8.0
Summary

CWNU 4190 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very 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=0.96) 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) 96.395 7.873 0.366 -0.051 -0.979 –
           
UCC 96.403 7.903 0.37 -0.072 -0.99 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4190 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.2, m-M=12.0, logA=7.5

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 3777 4.0 96.06 8.28 0.29 -0.1 -1.02 13.89 0.06