LISC-III 3411

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0.04 UTI
0.0
CN
0.05
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
N50 (P>50% members) 10
Stellar density (N50/rad) 0.3 [N/pc2]
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 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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LISC-III 3411 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a relatively close* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~1.22 kpc) differs significantly from the median photometric distance (~2.00 kpc).

⚠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.

Data
🔍 Search references for LISC-III 3411 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– 223.636 -57.505 0.817 -3.786 -3.024 -30.45
Chi et al. 2023 223.788 -57.487 0.94 -3.754 -3.03 –

💡 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– 2.0 2.0 – – 0.680 – 0.54 –
Chi et al. 2023 2.00 2.00 – – 0.680 – 0.54 –

Visualization
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LISC-III 3411 UCC
Galactocentric position diagram