LISC 3250

0.11 UTI

0.72

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.2

C_dup

N₅₀ (P>50% members) 93

Stellar density (N₅₀/rad) 13.6 [N/pc²]

C3 classification AA

C_N 0.72 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.2 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

LISC 3250 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is 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

Data

🔍 Search references for LISC 3250 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	216.2	-61.046	0.489	-3.738	-2.162	-0.03
Li et al.	2022	216.168	-61.041	0.492	-3.73	-2.105	–

💡 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–	2.0	1.82	–	–	-0.419	–	0.55	–
Li et al.	2022	2.00	1.82	–	–	-0.419	–	0.55	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 296	79.6	216.21	-61.04	0.48	-3.73	-2.19	-0.03	0.73
CWWDL 7479	50.5	216.2	-61.05	0.49	-3.75	-2.17	-64.97	0.0

💡 Note: The % column shows the percentage of members that LISC 3250 shares with each listed object.

Visualization

ℹ️