CWNU 3722

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.1 0.62 0.0 0.92
C3
N_50
r_50
AC 20 9.9
Summary

CWNU 3722 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate 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 very small percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.92) 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) 204.207 -63.609 0.454 -3.573 -1.677 –
           
UCC 204.137 -63.645 0.454 -3.617 -1.708 6.702
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3722 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.05, m-M=11.6, logA=6.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 3381 8.0 203.68 -63.33 0.47 -3.82 -1.63 – 0.45