CWNU 1487

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C3
N_50
r_50
CB 24 6.3
Summary

CWNU 1487 is a sparse, moderately dense object of low C3 quality. It is located at a relatively close 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 114.827 -14.729 0.643 -2.336 -0.292
Hunt & Reffert (2023) 114.812 -14.73 0.634 -2.331 -0.28 50.104
Cavallo et al. (2024) 114.841 -14.767 0.634
Hunt & Reffert (2024) 114.812 -14.73 0.634 -2.331 -0.28 50.104
Hu & Soubiran (2025) 114.841 -14.767
           
UCC 114.825 -14.742 0.64 -2.33 -0.283 43.894
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. (2023) A0=0.65, m-M=10.9, logAge=8.95
Hunt & Reffert (2023) AV50=0.522, diffAV50=0.397, MOD50=10.878, logAge50=8.702
Cavallo et al. (2024) AV50=1.01, dMod50=10.65, logAge50=8.81, [Fe/H]50=-0.54
Hunt & Reffert (2024) MassJ=63.3537, MassTot=137.659
Hu & Soubiran (2025) MA22=-0.1, MA23f=-0.15, MZ23=-0.05, MK24=-0.11, MF24=0.0

Search coordinates in Bayestar19

Cluster region map