LISC 3121

0.00 UTI

0.66

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 83

Stellar density (N₅₀/rad) 10.4 [N/pc²]

C3 classification AA

C_N 0.66 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC 3121 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old 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 Near-solar metallicity Old

Data

🔍 Search references for LISC 3121 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–	290.628	8.413	0.567	-1.339	-2.385	-4.706
Li et al.	2022	290.634	8.398	0.574	-1.323	-2.401	–

💡 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–	1.74	1.8	–	1600	-0.419	–	0.54	–
Li et al.	2022	1.74	1.80	–	1600	-0.419	–	0.54	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 119	100.0	290.63	8.42	0.57	-1.34	-2.38	-4.71	0.64
CWWDL 4494	72.3	290.62	8.42	0.57	-1.33	-2.38	-4.54	0.0

💡 Note: The % column shows the percentage of members that LISC 3121 shares with each listed object.

Visualization

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