LISC 1024

0.12 UTI

0.76

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.24

C_dup

C3 classification AB

Number of members (P>50%) 121

Radius (P>50% members) 3.9 [arcmin]

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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LISC 1024 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an extremely metal-poor, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~2.94 kpc) differs significantly from the median photometric distance (~1.74 kpc).

Relatively close Moderate extinction Extremely metal-poor Intermediate age

Data

🔍 Search references for LISC 1024 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	–	109.852	-21.417	0.34	-1.886	2.554	63.805
Li et al.	2022	109.855	-21.422	0.336	-1.871	2.701	–

💡 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
Li et al.	2022	1.74	1.30	–	100	-3.925	–	0.55	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 3524	76.0	109.85	-21.42	0.34	-1.89	2.53	81.64	0.03
UBC 457	76.0	109.85	-21.41	0.34	-1.88	2.51	49.83	0.65

💡 Note: The % column shows the percentage of members that LISC 1024 shares with each listed object.

Visualization

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