CWNU 3400

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C3
N_50
r_50
AB 48 1.7
Summary

CWNU 3400 is a poorly populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.

Warning: This is very likely a duplicate object, which shares a large 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) 282.99 -0.443 0.233 -0.98 -1.686 46.23
           
UCC 282.986 -0.443 0.23 -0.977 -1.69 46.131
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3400 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=5.35, m-M=12.6, logA=8.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 320 95.8 282.98 -0.44 0.23 -0.97 -1.69 46.13 0.55