CWNU 1585

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C3
N_50
r_50
DB 24 4.8
Summary

CWNU 1585 is a sparse, very loose object of low C3 quality. It is located at a moderate 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) 327.384 52.644 0.309 -2.839 -2.692
Hunt & Reffert (2023) 327.361 52.626 0.301 -2.81 -2.659 -51.107
Cavallo et al. (2024) 327.25 52.562 0.299
Hunt & Reffert (2024) 327.361 52.626 0.301 -2.81 -2.659 -51.107
           
UCC 327.38 52.61 0.309 -2.818 -2.685 -50.899
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=3.55, m-M=12.85, logAge=6.95
Hunt & Reffert (2023) AV50=3.128, diffAV50=1.821, MOD50=12.343, logAge50=7.878
Cavallo et al. (2024) AV50=3.12, dMod50=12.17, logAge50=8.2, [Fe/H]50=0.09
Hunt & Reffert (2024) MassJ=351.525, MassTot=473.876

Search coordinates in Bayestar19

Cluster region map