LISC 1145

0.27 UTI

0.81

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.52

C_dup

N₅₀ (P>50% members) 253

Stellar density (N₅₀/rad) 9.6 [N/pc²]

C3 classification AB

C_N 0.81 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.52 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC 1145 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

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 Low extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for LISC 1145 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–	114.523	-25.374	0.498	-2.628	3.201	48.708
Li et al.	2022	114.53	-25.402	0.516	-2.626	3.157	–

💡 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–	1.66	0.9	–	200	-0.419	–	0.51	–
Li et al.	2022	1.66	0.90	–	200	-0.419	–	0.51	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 230	47.8	114.52	-25.36	0.51	-2.63	3.2	39.44	0.68

💡 Note: The % column shows the percentage of members that LISC 1145 shares with each listed object.

Visualization

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