LISC 0896

0.03 UTI

0.76

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.07

C_dup

N₅₀ (P>50% members) 116

Stellar density (N₅₀/rad) 6.5 [N/pc²]

C3 classification AB

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 0.07 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC 0896 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich 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.

Relatively close Moderate extinction Metal-rich

Data

🔍 Search references for LISC 0896 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–	119.271	-22.806	0.385	-2.982	2.88	52.451
Li et al.	2022	119.265	-22.803	0.38	-2.957	2.889	–

💡 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–	2.75	1.02	–	–	0.680	–	0.5	–
Li et al.	2022	2.75	1.02	–	–	0.680	–	0.50	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 229	93.1	119.27	-22.8	0.38	-2.99	2.88	52.45	0.64
CWWDL 2972	54.3	119.26	-22.82	0.39	-2.97	2.87	38.0	0.0

💡 Note: The % column shows the percentage of members that LISC 0896 shares with each listed object.

Visualization

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