CWNU 1180

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C3
N_50
r_50
CC 24 39.7
Summary

CWNU 1180 is a sparse, loose object of low C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.

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

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. (2022) 272.573 -74.817 3.406 1.851 -14.3
           
UCC 272.046 -74.333 3.376 1.785 -14.414 20.243
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1180 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) A0=0.45, logAge=7.95

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 696 56.0 272.25 -73.6 3.38 1.43 -14.68 20.3 0.09