CWNU 1793

Click to load Aladin Lite
C3
N_50
r_50
DC 19 3.9
Summary

CWNU 1793 is a sparse, loose object of very low 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) 351.409 57.046 0.36 -2.396 -1.343 -35.26
           
UCC 351.414 57.046 0.356 -2.391 -1.319 -35.257
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1793 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.1, m-M=12.0, logAge=8.25

Search coordinates in Bayestar19

Cluster region map