LISC-III 3732

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0.07 UTI
0.0
CN
0.08
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
C3 classification CC
Number of members (P>50%) 16
Radius (P>50% members) 38.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique
📥 Members 📊 Colab 🔬 Bayestar19 🔍 SciX 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview
LISC-III 3732 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close* distance, above 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 (~0.58 kpc) differs significantly from the median photometric distance (~1.44 kpc).

⚠️ 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 Metal-rich

Data
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 293.231 28.712 1.727 0.845 -2.888 -21.102
Chi et al. 2023 292.847 28.995 1.886 0.792 -2.9 –

💡 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] Bfr BSS
Chi et al. 2023 1.44 1.75 – – 0.680 – 0.31 –

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.

Visualization
LISC-III 3732 UCC
Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.