CWNU 4815

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.03 0.38 0.0 1.0
C3
N_50
r_50
CB 16 3.7
Summary

CWNU 4815 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well above 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) 280.591 4.445 0.119 -2.283 -5.134 –
           
UCC 280.591 4.422 0.102 -2.332 -5.151 -0.688
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4815 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.9, m-M=13.45, logA=9.6

Search coordinates in Bayestar19

Cluster region map