CWNU 1449

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C3
N_50
r_50
CB 24 5.6
Summary

CWNU 1449 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below 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) 114.631 -27.809 0.354 -2.405 2.485
Hunt & Reffert (2023) 114.627 -27.914 0.341 -2.404 2.515
Cavallo et al. (2024) 114.582 -27.794 0.344
Hunt & Reffert (2024) 114.627 -27.914 0.341 -2.404 2.515
           
UCC 114.61 -27.809 0.34 -2.377 2.486
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=1.8, m-M=12.3, logAge=7.0
Hunt & Reffert (2023) AV50=1.545, diffAV50=1.64, MOD50=12.071, logAge50=7.713
Cavallo et al. (2024) AV50=1.51, dMod50=12.33, logAge50=7.67, [Fe/H]50=0.57
Hunt & Reffert (2024) MassJ=173.900, MassTot=170.317

Search coordinates in Bayestar19

Cluster region map