CWNU 4265

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C3
N_50
r_50
DC 59 4.9
Summary

CWNU 4265 is a moderately populated, very loose object of very low C3 quality. It is located at a large distance from the Sun, below 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 102.69 -3.591 0.168 -0.54 0.922
           
UCC 102.69 -3.589 0.165 -0.535 0.922 90.75
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4265 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.45, m-M=13.25, logA=7.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1706 45.8 102.69 -3.61 0.17 -0.51 0.9 105.34 0.28