LISC 2337

0.14 UTI

0.5

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.32

C_dup

N₅₀ (P>50% members) 50

Stellar density (N₅₀/rad) 16.7 [N/pc²]

C3 classification AB

C_N 0.5 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.32 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC 2337 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by low 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 (~2.29 kpc) differs significantly from the median photometric distance (~1.31 kpc).

Relatively close Low extinction Extremely metal-poor Intermediate age

Data

🔍 Search references for LISC 2337 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–	170.323	-60.557	0.437	-6.354	1.201	-3.783
Li et al.	2022	170.337	-60.568	0.43	-6.375	1.207	–

💡 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–	1.31	0.98	–	500	-2.721	–	0.54	–
Li et al.	2022	1.31	0.98	–	500	-2.721	–	0.54	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 2215	86.0	170.31	-60.56	0.44	-6.34	1.19	1.71	0.05
UBC 273	68.0	170.31	-60.56	0.43	-6.35	1.16	–	0.56

💡 Note: The % column shows the percentage of members that LISC 2337 shares with each listed object.

Visualization

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