CWNU 1796

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.04 0.12 0.0 1.0
C3
N_50
r_50
DC 15 12.0
Summary

CWNU 1796 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.

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

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) 309.381 47.64 0.428 -2.769 -4.715 –
           
UCC 309.416 47.576 0.417 -2.759 -4.718 -68.517
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1796 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.6, m-M=11.95, logAge=7.0

Search coordinates in Bayestar19

Cluster region map