CWNU 1075

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.24 0.38 0.0 1.0
C3
N_50
r_50
CB 22 42.3
Summary

CWNU 1075 is a sparse, very loose object of low C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It was recently reported in the literature.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 300.349 38.182 2.876 3.247 0.496 –
Hunt & Reffert (2023) 300.184 38.72 2.886 2.943 0.419 -17.909
Cavallo et al. (2024) 299.848 38.483 2.884 – – –
           
UCC 299.684 38.518 2.88 2.968 0.407 -19.984
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1075 UCC
CWNU 1075 HUNT23

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Fundamental parameters

Reference Values
He et al. (2022) A0=0.25, logAge=7.75
Hunt & Reffert (2023) AV50=0.132, diffAV50=0.578, MOD50=7.643, logAge50=8.071
Cavallo et al. (2024) AV50=0.7, dMod50=7.72, logAge50=7.73, [Fe/H]50=0.08

Search coordinates in Bayestar19

Cluster region map