CWNU 2157

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C3
N_50
r_50
DB 22 13.1
Summary

CWNU 2157 is a sparse, very loose object of low C3 quality. It is located at a relatively 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. (2023) 91.955 21.037 0.547 1.42 -2.435 61.28
Hunt & Reffert (2023) 91.916 21.025 0.549 1.447 -2.418
Cavallo et al. (2024) 92.107 21.031 0.551
           
UCC 91.959 21.01 0.547 1.426 -2.42 61.28
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. (2023) A0=1.4, m-M=11.4, logAge=6.95
Hunt & Reffert (2023) AV50=0.983, diffAV50=0.545, MOD50=11.133, logAge50=7.796
Cavallo et al. (2024) AV50=1.26, dMod50=11.38, logAge50=8.65, [Fe/H]50=-0.12

Search coordinates in Bayestar19

Cluster region map