CWNU 1433

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C3
N_50
r_50
DC 14 11.9
Summary

CWNU 1433 is a sparse, very loose object of very low 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 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) 38.03 56.474 0.36 -0.62 -0.484 -3.84
           
UCC 37.931 56.503 0.363 -0.63 -0.476
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1433 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.45, m-M=11.95, logAge=9.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1509 4.0 38.3 56.75 0.33 -0.79 -0.62 -44.2 0.06