LISC 3483

0.52 UTI

0.59

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 68

Radius (P>50% members) 5.1 [arcmin]

C_N 0.59 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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LISC 3483 is a moderately populated, very dense object of very 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 near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 3 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for LISC 3483 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	–	245.262	-40.836	0.905	-2.833	-3.385	-15.377
Li et al.	2022	245.282	-40.793	0.924	-2.877	-3.312	–

💡 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	1.04	2.45	–	100	-0.419	–	0.55	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 351	92.6	245.25	-40.84	0.91	-2.83	-3.39	-15.38	0.02
Theia 2501	89.7	245.25	-40.84	0.91	-2.84	-3.39	-15.38	0.0
OC 0667	50.0	245.25	-40.83	0.92	-2.85	-3.37	-15.38	0.0

💡 Note: The % column shows the percentage of members that LISC 3483 shares with each listed object.

Visualization

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