LISC 3316

0.01 UTI

0.56

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.03

C_dup

C3 classification AB

Number of members (P>50%) 63

Radius (P>50% members) 8.5 [arcmin]

C_N 0.56 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

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LISC 3316 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close^* distance, below the mid-plane, affected by low extinction. It is catalogued as a very metal-poor, 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.

(*): The parallax distance estimate (~1.43 kpc) differs significantly from the median photometric distance (~0.84 kpc).

Close Low extinction Very metal-poor Intermediate age

Data

🔍 Search references for LISC 3316 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	–	173.073	-68.08	0.698	-8.821	0.758	1.537
Li et al.	2022	173.08	-68.061	0.687	-8.836	0.774	–

💡 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	0.84	0.62	–	700	-1.335	–	0.49	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 16	96.8	173.13	-68.1	0.69	-8.82	0.75	1.54	0.47
CWWDL 14104	92.1	173.05	-68.08	0.7	-8.82	0.76	1.54	0.04
Theia 2982	81.0	173.12	-68.1	0.69	-8.82	0.75	1.54	0.02

💡 Note: The % column shows the percentage of members that LISC 3316 shares with each listed object.

Visualization

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