CWNU 1270

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C3
N_50
r_50
CC 23 33.0
Summary

CWNU 1270 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.

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) 343.1 51.337 2.121 3.084 0.051
Hunt & Reffert (2023) 344.047 50.869 2.115 3.187 0.112 2.66
Cavallo et al. (2024) 343.679 51.214 2.108
           
UCC 343.476 51.22 2.11 3.168 0.075 -0.423
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) A0=0.6, logAge=8.1
Hunt & Reffert (2023) AV50=0.034, diffAV50=0.232, MOD50=8.335, logAge50=7.979
Cavallo et al. (2024) AV50=0.71, dMod50=8.57, logAge50=7.18, [Fe/H]50=-0.54

Search coordinates in Bayestar19

Cluster region map