CWNU 2851

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C3
N_50
r_50
DC 30 6.1
Summary

CWNU 2851 is a poorly populated, very loose object of very low C3 quality. It is located at a moderate 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 2 later reported entries.

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) 357.018 68.269 0.353 -3.043 0.123
           
UCC 357.068 68.268 0.304 -3.026 0.092 -50.759
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2851 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.4, m-M=12.2, logAge=9.25

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3284 6.7 356.83 68.24 0.22 -2.5 -0.07 -75.19 0.08
HSC 936 3.3 356.83 68.25 0.21 -2.51 -0.06 -75.19 0.54