CWNU 320

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C3
N_50
r_50
AB 23 3.0
Summary

CWNU 320 is a sparse, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 109.93 -24.032 0.83 -2.75 3.06
He et al. (2022) 109.899 -24.033 0.822 -2.739 3.073
           
UCC 109.914 -24.039 0.83 -2.729 3.071 40.305
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 320 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=0.6, m-M=11.0, logAge=6.3, Z=0.008
He et al. (2022) A0=0.3, logAge=6.75

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0406 100.0 109.91 -24.04 0.83 -2.73 3.07 40.3 0.35