LISC 3479

0.02 UTI

0.64

C_N

0.13

C_dens

0.75

C_C3

0.0

C_lit

0.05

C_dup

N_m (P>50%) 77

Core radius and density 4.8 [pc], 0.7 [pc^-2]

C3 classification AB

C_N 0.64 Moderately populated
C_dens 0.13 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.05 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC 3479 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, 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.

Close Low extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for LISC 3479 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–	79.179	41.746	1.031	2.516	-4.706	-9.394
Li et al.	2022	79.233	41.735	1.029	2.505	-4.716	–

💡 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–	0.95	0.89	–	200	-0.259	–	0.42	–
Deng & Li	2023	0.95	0.89	–	200	-0.238	–	–	–
Li et al.	2022	0.95	0.89	–	200	-0.279	–	0.42	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
COIN-Gaia 12	94.8	79.18	41.75	1.03	2.52	-4.71	-8.95	0.58

💡 Note: The % column shows the percentage of members that LISC 3479 shares with each listed object.

Visualization

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