LISC 2967

0.24 UTI

0.27

C_N

0.16

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 27

Core radius and density 2.2 [pc], 0.8 [pc^-2]

C3 classification AB

C_N 0.27 Poorly populated
C_dens 0.16 Very loose
C_C3 0.75 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 2967 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for LISC 2967 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–	92.077	28.069	0.253	-0.176	-1.669	4.423
Li et al.	2022	92.06	28.062	0.273	-0.089	-1.618	–

💡 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–	3.805	1.04	–	650	0.127	–	0.54	–
Deng & Li	2023	3.63	1.11	–	700	-0.041	–	–	–
Li et al.	2022	3.98	0.97	–	600	0.295	–	0.54	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1295	88.9	92.08	28.07	0.26	-0.2	-1.69	0.53	0.16
CWWDL 2957	77.8	92.08	28.07	0.26	-0.16	-1.69	4.42	0.03

💡 Note: The % column shows the percentage of members that LISC 2967 shares with each listed object.

Visualization

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