LISC 3530

0.09 UTI

0.71

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.17

C_dup

C3 classification AB

Number of members (P>50%) 92

Radius (P>50% members) 19.1 [arcmin]

C_N 0.71 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.17 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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LISC 3530 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close^* distance, below the mid-plane, affected by low extinction. It is catalogued as a very metal-poor, intermediate-age 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.

(*): The parallax distance estimate (~0.51 kpc) differs significantly from the median photometric distance (~0.38 kpc).

Very close Low extinction Very metal-poor Intermediate age

Data

🔍 Search references for LISC 3530 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	–	277.296	-34.539	1.968	1.181	-8.664	-0.001
Li et al.	2022	277.339	-34.579	1.954	1.204	-8.724	–

💡 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	0.38	0.50	–	200	-1.335	–	0.33	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 654	82.6	277.3	-34.54	1.97	1.19	-8.67	0.65	0.79

💡 Note: The % column shows the percentage of members that LISC 3530 shares with each listed object.

Visualization

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