CWNU 4355

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C3
N_50
r_50
CB 17 6.2
Summary

CWNU 4355 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 342.898 57.932 0.28 -3.274 -2.553
           
UCC 342.936 57.958 0.277 -3.277 -2.528
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4355 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.5, m-M=12.6, logA=7.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 837 80.0 342.97 58.02 0.28 -3.24 -2.49 -79.96 0.29