CWNU 1087

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C3
N_50
r_50
AB 33 10.0
Summary

CWNU 1087 is a poorly populated, dense object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a small percentage of members with a later reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 113.044 -14.107 1.016 -2.376 0.399
Hunt & Reffert (2023) 113.073 -14.072 0.974 -2.398 0.457 25.889
Cavallo et al. (2024) 113.022 -14.078 0.988
Hunt & Reffert (2024) 113.073 -14.072 0.974 -2.398 0.457 25.889
           
UCC 113.059 -14.06 0.992 -2.374 0.423 27.21
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) A0=0.35, logAge=8.85
Hunt & Reffert (2023) AV50=0.166, diffAV50=0.326, MOD50=9.898, logAge50=8.224
Cavallo et al. (2024) AV50=0.6, dMod50=9.96, logAge50=8.2, [Fe/H]50=-0.3
Hunt & Reffert (2024) MassJ=61.0884, MassTot=71.0504

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14462 15.2 113.07 -14.09 0.86 -2.77 0.56 24.55 0.05