LISC-III 1911

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0.09 UTI
0.0
CN
0.06
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
N50 (P>50% members) 15
Radius (P>50% members) 10.1 [arcmin]
C3 classification BC
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.38 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 1911 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity 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.

Relatively close Moderate extinction Near-solar metallicity

Data
🔍 Search references for LISC-III 1911 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– 75.512 20.923 0.407 0.811 -1.789 14.861
Chi et al. 2023 75.543 20.921 0.472 0.882 -1.827 –

💡 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– 2.19 1.2 – – 0.274 – 0.52 –
Chi et al. 2023 2.19 1.20 – – 0.274 – 0.52 –

Visualization
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LISC-III 1911 UCC
Galactocentric position diagram