CWNU 4778

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C3
N_50
r_50
BB 24 31.0
Summary

CWNU 4778 is a sparse, very loose object of intermediate C3 quality. It is located at a close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This is likely a unique object, which shares a moderate 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) 23.198 67.178 1.58 -5.68 -0.487 -24.31
           
UCC 24.141 67.218 1.607 -5.68 -0.495 -23.508
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4778 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.95, m-M=9.0, logA=7.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 850 36.0 26.5 66.91 1.61 -5.6 -0.34 -19.94 0.26