CWNU 1625

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C3
N_50
r_50
BB 23 6.3
Summary

CWNU 1625 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, above 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) 341.965 62.447 0.28 -2.969 -1.463
Hunt & Reffert (2023) 341.953 62.463 0.265 -3.01 -1.464 8.192
Cavallo et al. (2024) 342.01 62.427 0.273
Hunt & Reffert (2024) 341.953 62.463 0.265 -3.01 -1.464 8.192
           
UCC 341.954 62.433 0.269 -2.988 -1.455 8.194
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=4.15, m-M=13.15, logAge=6.6
Hunt & Reffert (2023) AV50=3.726, diffAV50=1.876, MOD50=12.653, logAge50=7.166
Cavallo et al. (2024) AV50=3.25, dMod50=12.26, logAge50=7.74, [Fe/H]50=0.35
Hunt & Reffert (2024) MassJ=253.653, MassTot=415.266

Search coordinates in Bayestar19

Cluster region map