CWNU 3444

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C3
N_50
r_50
CB 22 6.2
Summary

CWNU 3444 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It was recently reported in the literature.

Warning: This is possibly a duplicated object, which shares a significant 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) 113.596 -13.62 0.2 -1.374 1.836 90.31
           
UCC 113.594 -13.649 0.2 -1.372 1.868 77.28
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3444 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.75, m-M=13.2, logA=8.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1814 68.0 113.52 -13.61 0.2 -1.37 1.87 90.31 0.12
ASCC 40 36.0 113.43 -13.77 0.18 -1.38 1.74 95.1 0.32