CWNU 3837

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C3
N_50
r_50
CB 34 5.0
Summary

CWNU 3837 is a poorly populated, very loose object of low C3 quality. It is located at a large distance from the Sun, well above 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: 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) 320.261 57.252 0.129 -2.448 -2.235 -83.58
           
UCC 320.278 57.256 0.136 -2.476 -2.254 -82.981
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3837 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=3.25, m-M=13.6, logA=8.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3895 5.9 320.71 57.13 0.13 -2.38 -2.09 -98.29 0.05