CWNU 3450

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.05 0.38 0.0 0.4
C3
N_50
r_50
CB 20 3.1
Summary

CWNU 3450 is a sparse, very loose object of low C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It was recently reported in the literature.

Warning: This is possibly a duplicated object, which shares a significant 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) 105.305 -15.163 0.101 -0.253 1.276 –
           
UCC 105.304 -15.154 0.097 -0.282 1.285 63.438
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3450 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.8, m-M=14.1, logA=8.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1794 60.0 105.31 -15.16 0.1 -0.26 1.28 – 0.26