LISC 3180

0.05 UTI

0.75

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.09

C_dup

C3 classification AA

Number of members (P>50%) 113

Radius (P>50% members) 3.2 [arcmin]

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 0.09 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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LISC 3180 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate 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.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for LISC 3180 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	–	259.286	-41.524	0.548	0.088	-0.76	1.781
Li et al.	2022	259.293	-41.518	0.54	0.109	-0.785	–

💡 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]	Bfr	BSS
Li et al.	2022	1.66	2.50	–	700	-0.419	–	0.51	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 556	91.2	259.29	-41.53	0.55	0.09	-0.75	41.82	0.75

💡 Note: The % column shows the percentage of members that LISC 3180 shares with each listed object.

Visualization

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