CWNU 1817

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.28 0.62 0.0 1.0
C3
N_50
r_50
AC 20 5.8
Summary

CWNU 1817 is a sparse, loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, below 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) 168.57 -62.833 0.441 -7.512 1.699 –
           
UCC 168.602 -62.852 0.443 -7.495 1.702 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1817 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.65, m-M=11.85, logAge=7.1

Search coordinates in Bayestar19

Cluster region map