LISC 2425

0.04 UTI

0.77

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.08

C_dup

N₅₀ (P>50% members) 153

Stellar density (N₅₀/rad) 19.2 [N/pc²]

C3 classification AB

C_N 0.77 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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LISC 2425 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by high extinction. It is catalogued as an extremely metal-poor, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very 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 (~2.37 kpc) differs significantly from the median photometric distance (~1.20 kpc).

Relatively close High extinction Extremely metal-poor Intermediate age

Data

🔍 Search references for LISC 2425 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–	235.716	-55.417	0.422	-3.813	-3.974	-46.732
Li et al.	2022	235.721	-55.402	0.434	-3.812	-3.978	–

💡 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]	B_frac	BSS
UCC	99999–	1.2	3.73	–	900	-3.925	–	0.53	–
Li et al.	2022	1.20	3.73	–	900	-3.925	–	0.53	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UFMG 43	91.5	235.72	-55.42	0.41	-3.83	-3.95	-46.73	0.61

💡 Note: The % column shows the percentage of members that LISC 2425 shares with each listed object.

Visualization

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