CWNU 1417

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C3
N_50
r_50
CA 30 2.5
Summary

CWNU 1417 is a poorly populated, loose 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 165.2 -61.629 0.161 -6.072 2.509 24.34
           
UCC 165.205 -61.621 0.157 -6.072 2.52 23.421
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1417 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.55, m-M=13.65, logAge=8.65

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch J1059.7-6131 86.7 165.11 -61.59 0.14 -6.1 2.54 24.22 0.3