CWNU 2790

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.08 0.12 0.0 1.0
C3
N_50
r_50
DC 14 6.0
Summary

CWNU 2790 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) 123.558 -30.654 0.302 -1.97 2.312 –
           
UCC 123.581 -30.635 0.291 -1.995 2.317 70.709
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2790 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.35, m-M=12.65, logAge=9.5

Search coordinates in Bayestar19

Cluster region map