LISC 0988

0.04 UTI

0.75

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.09

C_dup

N₅₀ (P>50% members) 105

Stellar density (N₅₀/rad) 20.8 [N/pc²]

C3 classification AB

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.09 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC 0988 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for LISC 0988 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–	83.771	15.72	0.7	0.254	-2.393	10.424
Li et al.	2022	83.749	15.748	0.695	0.254	-2.377	–

💡 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–	1.45	1.9	–	100	-0.419	–	0.54	–
Li et al.	2022	1.45	1.90	–	100	-0.419	–	0.54	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
COIN-Gaia 26	91.4	83.77	15.72	0.7	0.25	-2.4	10.42	0.81
UBC 75	90.5	83.77	15.72	0.7	0.26	-2.4	10.42	0.03
CWWDL 3284	83.8	83.77	15.72	0.7	0.25	-2.39	10.42	0.0

💡 Note: The % column shows the percentage of members that LISC 0988 shares with each listed object.

Visualization

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