LISC 1314

0.55 UTI

0.76

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 130

Stellar density (N₅₀/rad) 9.4 [N/pc²]

C3 classification AA

C_N 0.76 Rich
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

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

Overview

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LISC 1314 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a very metal-poor, old cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~3.36 kpc) differs significantly from the median photometric distance (~2.29 kpc).

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

Relatively close Moderate extinction Very metal-poor Old

Data

🔍 Search references for LISC 1314 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–	222.559	-61.766	0.297	-3.445	-1.918	-33.636
Li et al.	2022	222.561	-61.78	0.295	-3.438	-1.914	–

💡 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–	2.29	2.5	–	1000	-1.335	–	0.54	–
Li et al.	2022	2.29	2.50	–	1000	-1.335	–	0.54	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1532	99.2	222.56	-61.76	0.3	-3.45	-1.92	-33.64	0.06
CWWDL 913	48.5	222.55	-61.76	0.3	-3.44	-1.91	-34.03	0.0
OC 0614	19.2	222.55	-61.76	0.3	-3.43	-1.9	-34.03	0.0

💡 Note: The % column shows the percentage of members that LISC 1314 shares with each listed object.

Visualization

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