CWNU 1778

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.26 0.11 0.38 0.0 1.0
C3
N_50
r_50
BC 26 16.6
Summary

CWNU 1778 is a poorly populated, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a moderate percentage of members with a later reported entry.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) 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) 101.905 -13.421 0.702 -2.924 2.058 –
           
UCC 101.854 -13.327 0.705 -2.905 2.079 89.526
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1778 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.9, m-M=10.7, logAge=7.45

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 1769 42.3 101.91 -12.98 0.71 -2.93 2.06 42.34 0.08