CWNU 3477

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C3
N_50
r_50
AC 90 2.7
Summary

CWNU 3477 is a moderately populated, loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well above 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 340.27 64.15 0.1 -2.6 -1.259
           
UCC 340.278 64.155 0.1 -2.585 -1.246
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3477 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.0, m-M=14.75, logA=7.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 857 35.6 340.27 64.15 0.11 -2.59 -1.24 0.35