LISC 3106

0.00 UTI

0.53

C_N

0.88

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 56

Stellar density (N₅₀/rad) 4.4 [N/pc²]

C3 classification AB

C_N 0.53 Moderately populated
C_dens 0.88 Dense
C_C3 0.75 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 3106 is a moderately populated, 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 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 (~2.08 kpc) differs significantly from the median photometric distance (~1.38 kpc).

Relatively close Moderate extinction Extremely metal-poor Intermediate age

Data

🔍 Search references for LISC 3106 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–	100.0	-3.638	0.482	0.09	-0.423	24.665
Li et al.	2022	100.016	-3.673	0.489	0.115	-0.433	–

💡 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–	1.38	1.25	–	200	-2.721	–	0.5	–
Li et al.	2022	1.38	1.25	–	200	-2.721	–	0.50	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 441	100.0	99.98	-3.63	0.48	0.08	-0.41	24.66	0.62
CWWDL 128	94.6	99.98	-3.64	0.48	0.08	-0.43	19.67	0.01

💡 Note: The % column shows the percentage of members that LISC 3106 shares with each listed object.

Visualization

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