CWNU 136

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C3
N_50
r_50
AB 34 23.1
Summary

CWNU 136 is a poorly populated, very loose object of high C3 quality. It is located at a close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry, and a significant percentage with at least one entry reported in the same catalogue.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 310.932 56.496 1.1 -2.38 -5.04
Hunt & Reffert (2023) 311.219 56.9 1.091 -2.358 -4.97 -18.542
Cavallo et al. (2024) 311.038 56.78 1.093
Hunt & Reffert (2024) 311.219 56.9 1.091 -2.358 -4.97 -18.542
           
UCC 310.988 56.816 1.093 -2.343 -5.012 -9.865
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=1.9, m-M=9.7, logAge=7.5, Z=0.024
Hunt & Reffert (2023) AV50=1.399, diffAV50=2.267, MOD50=9.714, logAge50=6.967
Cavallo et al. (2024) AV50=2.39, dMod50=10.03, logAge50=6.96, [Fe/H]50=-0.23
Hunt & Reffert (2024) MassJ=87.0317, MassTot=235.031

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 521 64.7 310.55 56.87 1.09 -2.33 -5.02 -12.51 0.24
UPK 147 8.8 313.58 56.49 1.13 -2.4 -4.86 -16.72 0.14