CWNU 2025

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C3
N_50
r_50
BB 18 7.2
Summary

CWNU 2025 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.

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) 265.783 -44.972 0.48 -0.295 -3.709 1.81
           
UCC 265.836 -44.995 0.434 -0.302 -3.701
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2025 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.05, m-M=11.9, logAge=9.25

Search coordinates in Bayestar19

Cluster region map