LISC 1753

0.01 UTI

0.71

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.01

C_dup

N₅₀ (P>50% members) 92

Stellar density (N₅₀/rad) 19.2 [N/pc²]

C3 classification AA

C_N 0.71 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.01 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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LISC 1753 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 metal-rich, 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 Metal-rich Intermediate age

Data

🔍 Search references for LISC 1753 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–	242.894	-53.037	0.306	-2.485	-2.032	-64.678
Li et al.	2022	242.919	-53.034	0.3	-2.428	-2.068	–

💡 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–	2.75	2.17	–	900	0.680	–	0.53	–
Li et al.	2022	2.75	2.17	–	900	0.680	–	0.53	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 537	98.9	242.89	-53.04	0.3	-2.49	-2.02	-64.75	0.69
OC 0643	29.3	242.89	-53.04	0.3	-2.5	-2.03	-64.75	0.0

💡 Note: The % column shows the percentage of members that LISC 1753 shares with each listed object.

Visualization

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