CWNU 4615

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C3
N_50
r_50
CC 16 6.3
Summary

CWNU 4615 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a very small percentage of members with at least one entry reported in the same catalogue.

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) 333.269 60.83 0.123 -2.382 -1.814 -78.05
           
UCC 333.225 60.831 0.159 -2.405 -1.813 -73.566
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4615 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.9, m-M=14.35, logA=8.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4153 8.0 333.2 61.05 0.16 -2.41 -1.88 -78.26 0.09