CWNU 1295

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C3
N_50
r_50
AB 44 2.2
Summary

CWNU 1295 is a poorly populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.

Warning: This is possibly a duplicated object, which shares a significant 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. (2023) 92.078 28.071 0.283 -0.196 -1.683 8.32
Hunt & Reffert (2023) 92.082 28.073 0.256 -0.216 -1.668 7.407
Cavallo et al. (2024) 92.068 28.063 0.256
Hunt & Reffert (2024) 92.082 28.073 0.256 -0.216 -1.668 7.407
Hu & Soubiran (2025) 92.068 28.063
           
UCC 92.077 28.074 0.256 -0.198 -1.693 0.528
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=1.3, m-M=13.0, logAge=8.45
Hunt & Reffert (2023) AV50=0.864, diffAV50=1.549, MOD50=12.749, logAge50=8.748
Cavallo et al. (2024) AV50=1.19, dMod50=12.42, logAge50=8.75, [Fe/H]50=-0.35
Hunt & Reffert (2024) MassJ=519.575, MassTot=627.032
Hu & Soubiran (2025) MA22=-0.25, MA23f=-0.43, MA23g=-0.42, MZ23=-0.36, MK24=-0.3, MF24=-0.38

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
LISC 2967 54.5 92.08 28.07 0.25 -0.18 -1.67 4.42 0.36
CWWDL 2957 47.7 92.08 28.07 0.26 -0.16 -1.69 4.42 0.04