CWNU 3336

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 1.0 0.25 0.0 0.92
C3
N_50
r_50
DB 24 0.9
Summary

CWNU 3336 is a sparse, very dense object of low C3 quality. It is located at a large distance from the Sun, below 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) 130.887 -45.185 0.127 -3.102 3.344 89.53
           
UCC 130.888 -45.192 0.131 -3.139 3.345 89.531
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3336 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.65, m-M=15.85, logA=6.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch J0843.6-4511 8.0 130.9 -45.18 0.14 -3.38 3.2 49.06 0.09