CWNU 4132

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C3
N_50
r_50
DA 24 1.5
Summary

CWNU 4132 is a sparse, very dense object of intermediate 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.

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) 112.75 -18.916 0.262 -1.999 2.358
           
UCC 112.75 -18.93 0.269 -1.988 2.357
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4132 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.75, m-M=12.8, logA=7.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1853 92.0 112.75 -18.93 0.26 -1.99 2.35 0.48