CWNU 3187

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C3
N_50
r_50
AB 23 5.1
Summary

CWNU 3187 is a sparse, loose object of high C3 quality. It is located at a moderate distance from the Sun, above 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) 114.391 -18.063 0.36 -1.844 2.259
           
UCC 114.392 -18.063 0.361 -1.844 2.268
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3187 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.5, m-M=12.45, logA=7.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1854 84.0 114.39 -18.09 0.36 -1.84 2.27 0.28