LISC 3205

0.13 UTI

0.57

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.25

C_dup

N₅₀ (P>50% members) 64

Stellar density (N₅₀/rad) 5.9 [N/pc²]

C3 classification AA

C_N 0.57 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.25 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC 3205 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as an extremely metal-poor, 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.

(*): The parallax distance estimate (~2.26 kpc) differs significantly from the median photometric distance (~1.26 kpc).

Relatively close Moderate extinction Extremely metal-poor Intermediate age

Data

🔍 Search references for LISC 3205 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–	327.771	52.982	0.442	-4.122	-4.542	-31.635
Li et al.	2022	327.775	52.99	0.454	-4.124	-4.553	–

💡 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–	1.26	2.05	–	400	-2.721	–	0.54	–
Li et al.	2022	1.26	2.05	–	400	-2.721	–	0.54	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 1939	79.7	327.78	52.99	0.44	-4.13	-4.53	–	0.0
UBC 162	75.0	327.77	52.99	0.44	-4.12	-4.53	–	0.67

💡 Note: The % column shows the percentage of members that LISC 3205 shares with each listed object.

Visualization

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