CWNU 4102

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C3
N_50
r_50
BB 20 3.0
Summary

CWNU 4102 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 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) 270.086 -24.298 0.472 0.084 -1.116 92.36
           
UCC 270.06 -24.291 0.472 0.091 -1.147 37.838
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4102 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=3.05, m-M=11.9, logA=6.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 79 76.0 270.06 -24.29 0.48 0.09 -1.18 92.36 0.34
Ryu 596 4.0 270.22 -24.23 0.39 0.06 -1.42 25.14 0.22