CWNU 1024

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.8 1.0 1.0 0.25 1.0
C3
N_50
r_50
AA 239 56.6
Summary

CWNU 1024 is a rich, very dense object of very high C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with 2 later reported entries.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 104.451 -26.85 2.521 -6.046 6.01 –
Hunt & Reffert (2023) 104.286 -27.392 2.495 -5.545 6.018 21.594
Cavallo et al. (2024) 103.156 -25.587 2.497 – – –
           
UCC 104.396 -26.866 2.514 -6.018 6.017 21.44
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1024 UCC
CWNU 1024 HUNT23

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Fundamental parameters

Reference Values
He et al. (2022) A0=0.35, logAge=7.6
Hunt & Reffert (2023) AV50=0.173, diffAV50=0.732, MOD50=7.98, logAge50=7.511
Cavallo et al. (2024) AV50=0.43, dMod50=8.09, logAge50=7.05, [Fe/H]50=-0.16

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 144 93.7 104.27 -26.59 2.52 -6.01 6.01 21.57 0.07
CWWDL 14577 12.6 104.14 -26.7 2.57 -6.11 6.04 20.68 0.0