CWNU 3174

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C3
N_50
r_50
CA 21 0.9
Summary

CWNU 3174 is a sparse, very dense object of intermediate C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: This is likely a duplicate object, which shares a large 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) 126.103 -39.941 0.168 -2.587 3.226 207.08
           
UCC 126.107 -39.94 0.177 -2.602 3.236 207.082
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3174 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=5.0, m-M=14.55, logA=6.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 1387 80.0 126.1 -39.94 0.18 -2.59 3.28 207.08 0.43