LISC-III 932

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0.03 UTI
0.0
CN
0.05
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
N50 (P>50% members) 15
Radius (P>50% members) 6.0 [arcmin]
C3 classification DC
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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LISC-III 932 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a metal-rich cluster (see Parameters). It was recently reported in the literature.

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

Distant Low extinction Metal-rich

Data
🔍 Search references for LISC-III 932 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 104.007 10.407 0.217 -0.376 -0.617 85.022
Chi et al. 2023 104.01 10.402 0.245 -0.385 -0.602 –

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 4.79 0.2 – – 0.680 – 0.34 –
Chi et al. 2023 4.79 0.20 – – 0.680 – 0.34 –

Visualization
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LISC-III 932 UCC
Galactocentric position diagram