CWNU 3590

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.34 0.34 0.75 0.0 0.5
C3
N_50
r_50
AB 34 1.0
Summary

CWNU 3590 is a poorly populated, loose object of high 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.

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) 103.516 -13.566 0.053 -0.351 0.741 –
           
UCC 103.515 -13.567 0.065 -0.34 0.741 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3590 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.85, m-M=14.85, logA=8.1

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
DC 4 50.0 103.51 -13.57 0.11 -0.36 0.74 96.7 0.2