CWNU 3364

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.91 0.75 0.0 0.04
C3
N_50
r_50
AB 22 1.3
Summary

CWNU 3364 is a sparse, very dense object of high 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 very 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) 163.246 -61.286 0.168 -4.862 1.791 2.07
           
UCC 163.257 -61.286 0.172 -4.881 1.79 2.072
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3364 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.6, m-M=13.3, logA=7.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2392 96.0 163.26 -61.29 0.17 -4.88 1.79 2.07 0.42