LISC 3241

0.19 UTI

0.79

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.37

C_dup

N₅₀ (P>50% members) 196

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

C3 classification AB

C_N 0.79 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.37 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC 3241 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

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

Relatively close Moderate extinction Metal-rich Intermediate age

Data

🔍 Search references for LISC 3241 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–	174.025	-59.468	0.522	-6.497	1.656	-14.081
Li et al.	2022	174.002	-59.483	0.511	-6.512	1.67	–

💡 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–	1.82	1.02	–	100	0.680	–	0.45	–
Li et al.	2022	1.82	1.02	–	100	0.680	–	0.45	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 277	63.3	174.04	-59.47	0.53	-6.5	1.65	-16.12	0.64
CWWDL 13971	38.3	174.04	-59.49	0.52	-6.48	1.66	-16.12	0.0

💡 Note: The % column shows the percentage of members that LISC 3241 shares with each listed object.

Visualization

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