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

C3 classification AB

Number of members (P>50%) 105

Radius (P>50% members) 5.4 [arcmin]

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

Overview

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

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	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]	Bfr	BSS
Li et al.	2022	1.45	1.90	–	100	-0.419	–	0.54	–

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.

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	0.77
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

💡 Note: How are the galactocentric plots generated? See FAQ.