CWNU 3701

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.26 0.17 0.12 0.0 0.85
C3
N_50
r_50
DC 26 3.7
Summary

CWNU 3701 is a poorly populated, very loose object of very low C3 quality. It is located at a large distance from the Sun, near the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.85) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 141.96 -52.011 0.181 -4.461 3.456 –
           
UCC 141.992 -52.008 0.193 -4.44 3.421 32.954
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3701 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.8, m-M=13.45, logA=8.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2224 15.4 142.13 -52.12 0.21 -4.32 3.39 6.28 0.18