CWNU 48

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C3
N_50
r_50
CC 23 30.0
Summary

CWNU 48 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.

This is likely a unique object, which shares a moderate 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. (2022) 100.293 -23.789 0.96 -1.34 2.34
           
UCC 100.27 -23.829 0.975 -1.392 2.393 30.355
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 48 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=1.35, m-M=10.7, logAge=7.4, Z=0.002

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 69 32.0 101.15 -24.3 0.96 -1.52 2.46 36.01 0.47
Theia 3740 24.0 101.17 -24.29 0.96 -1.52 2.46 36.4 0.01