CWNU 2655

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C3
N_50
r_50
DC 24 8.9
Summary

CWNU 2655 is a sparse, very 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.

This is likely a unique object, which shares a moderate 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. (2023) 97.654 3.07 0.391 -0.269 -0.999 38.65
           
UCC 97.663 2.995 0.367 -0.278 -0.963
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2655 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.35, m-M=12.35, logAge=6.2

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Collinder 96 48.0 97.59 2.86 0.35 -0.24 -0.93 40.24 0.31