CWNU 394

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C3
N_50
r_50
BB 48 17.3
Summary

CWNU 394 is a poorly populated, loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, near 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, and a moderate percentage with at least one entry reported in the same catalogue.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 348.324 57.527 0.92 0.27 -1.37 -24.5
He et al. (2022) 348.051 57.538 0.913 0.225 -1.33
           
UCC 348.155 57.483 0.917 0.25 -1.351 -27.344
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 394 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=1.55, m-M=10.25, logAge=7.8, Z=0.038
He et al. (2022) A0=2.25, logAge=7.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14366 100.0 348.22 57.48 0.92 0.24 -1.34 -29.86 0.02
LISC 3420 54.2 348.1 57.47 0.91 0.26 -1.37 -31.89 0.24
Theia 2526 52.1 348.12 57.48 0.91 0.27 -1.37 -31.89 0.0
CWNU 415 47.9 347.86 57.41 0.91 0.24 -1.38 -23.5 0.04
CWNU 83 20.8 347.51 57.0 0.91 0.19 -1.4 -19.28 0.05