LISC 3315

0.10 UTI

0.75

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.18

C_dup

N₅₀ (P>50% members) 108

Stellar density (N₅₀/rad) 14.7 [N/pc²]

C3 classification AA

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.18 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC 3315 is a rich, 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 metal-poor, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

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

Close Moderate extinction Metal-poor Intermediate age

Data

🔍 Search references for LISC 3315 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–	126.669	-50.727	0.879	-5.047	6.176	17.871
Li et al.	2022	126.624	-50.693	0.891	-5.038	6.2	–

💡 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–	0.99	1.27	–	200	-0.642	–	0.55	–
Li et al.	2022	0.99	1.27	–	200	-0.642	–	0.55	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 247	81.5	126.67	-50.73	0.88	-5.05	6.17	17.87	0.79

💡 Note: The % column shows the percentage of members that LISC 3315 shares with each listed object.

Visualization

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