LISC 0672

0.25 UTI

0.77

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.5

C_dup

N₅₀ (P>50% members) 148

Stellar density (N₅₀/rad) 10.2 [N/pc²]

C3 classification AB

C_N 0.77 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.5 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC 0672 is a rich, very dense 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 an extremely metal-poor, old cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~3.63 kpc) differs significantly from the median photometric distance (~1.91 kpc).

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Extremely metal-poor Old

Data

🔍 Search references for LISC 0672 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–	192.618	-60.995	0.275	-6.518	-0.757	-33.021
Li et al.	2022	192.65	-60.993	0.274	-6.418	-0.722	–

💡 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–	1.91	1.75	–	1800	-5.024	–	0.4	–
Li et al.	2022	1.91	1.75	–	1800	-5.024	–	0.40	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 2772	78.4	192.62	-61.0	0.28	-6.52	-0.76	-31.33	0.0
UBC 524	50.0	192.62	-60.99	0.28	-6.56	-0.79	-25.76	0.73

💡 Note: The % column shows the percentage of members that LISC 0672 shares with each listed object.

Visualization

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