CWNU 3415

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C3
N_50
r_50
DC 30 3.8
Summary

CWNU 3415 is a poorly populated, very loose object of very low 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) 79.848 33.651 0.187 0.882 -0.008 -10.55
           
UCC 79.867 33.646 0.195 0.882 -0.008 -10.549
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3415 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.1, m-M=13.2, logA=8.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1353 76.7 79.86 33.65 0.2 0.88 -0.01 -10.55 0.22