CWNU 1092

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.28 0.21 0.38 0.0 1.0
C3
N_50
r_50
BC 28 41.9
Summary

CWNU 1092 is a poorly populated, 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: 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) 90.53 8.416 2.42 -3.299 -4.13 –
Hunt & Reffert (2023) 90.831 8.559 2.382 -3.397 -4.069 30.299
Cavallo et al. (2024) 90.892 8.239 2.383 – – –
           
UCC 90.857 8.345 2.369 -3.378 -4.042 30.104
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1092 UCC
CWNU 1092 HUNT23

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Fundamental parameters

Reference Values
He et al. (2022) A0=0.3, logAge=7.2
Hunt & Reffert (2023) AV50=0.13, diffAV50=0.412, MOD50=7.999, logAge50=7.276
Cavallo et al. (2024) AV50=0.65, dMod50=8.16, logAge50=7.33, [Fe/H]50=0.36

Search coordinates in Bayestar19

Cluster region map