CWNU 1045

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C3
N_50
r_50
CC 21 41.9
Summary

CWNU 1045 is a sparse, very loose object of low C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It was recently reported in the literature.

This object shares a very small 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) 314.54 46.539 2.665 5.671 0.984
           
UCC 314.269 46.3 2.674 5.804 1.215 -11.913
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1045 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) A0=0.45, logAge=7.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 693 8.0 314.61 47.44 2.6 4.72 0.54 -6.33 0.26