CWNU 114

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C3
N_50
r_50
BB 25 5.3
Summary

CWNU 114 is a poorly populated, moderately dense object of intermediate 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: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 29.319 63.153 0.55 0.09 -0.19
Hunt & Reffert (2023) 29.39 63.198 0.537 0.035 -0.214 -33.419
Cavallo et al. (2024) 29.31 63.161 0.548
Hunt & Reffert (2024) 29.39 63.198 0.537 0.035 -0.214 -33.419
           
UCC 29.378 63.176 0.556 0.078 -0.203 -33.418
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. (2022) AG=1.4, m-M=10.65, logAge=8.7, Z=0.004
Hunt & Reffert (2023) AV50=1.54, diffAV50=0.879, MOD50=11.149, logAge50=8.245
Cavallo et al. (2024) AV50=1.86, dMod50=11.69, logAge50=8.03, [Fe/H]50=0.59
Hunt & Reffert (2024) MassJ=155.490, MassTot=149.144

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1606 88.0 29.38 63.17 0.56 0.08 -0.23 -33.42 0.26