CWNU 2722

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C3
N_50
r_50
AB 26 9.1
Summary

CWNU 2722 is a poorly populated, very loose object of high C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a small percentage of members with a later reported entry.

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) 280.603 -11.291 0.563 0.657 -0.818
           
UCC 280.56 -11.333 0.562 0.66 -0.823 13.845
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2722 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.0, m-M=11.1, logAge=7.5

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 224 11.5 280.24 -11.76 0.56 0.67 -0.71 0.25