CWNU 1265

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C3
N_50
r_50
CB 29 48.5
Summary

CWNU 1265 is a poorly populated, 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.

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) 112.259 -48.755 3.819 -11.99 7.473
Hunt & Reffert (2023) 113.288 -49.138 3.834 -12.229 7.504 12.597
Cavallo et al. (2024) 112.43 -48.258 3.835
           
UCC 112.803 -48.833 3.807 -12.017 7.462 10.65
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

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Fundamental parameters

Reference Values
He et al. (2022) A0=0.8, logAge=7.65
Hunt & Reffert (2023) AV50=0.36, diffAV50=0.538, MOD50=7.067, logAge50=9.064
Cavallo et al. (2024) AV50=0.29, dMod50=7.12, logAge50=7.3, [Fe/H]50=-0.03

Search coordinates in Bayestar19

Cluster region map