CWNU 2679

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C3
N_50
r_50
BB 20 10.8
Summary

CWNU 2679 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a significant percentage of members with a later 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=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) 107.522 -15.259 0.352 -0.919 1.368 60.57
           
UCC 107.46 -15.176 0.349 -0.927 1.374
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2679 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.3, m-M=12.1, logAge=7.5

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1801 60.0 107.39 -15.03 0.33 -0.94 1.39 55.45 0.09