LISC-III 3613

0.14 UTI

0.62

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.27

C_dup

C3 classification AA

Number of members (P>50%) 74

Radius (P>50% members) 27.6 [arcmin]

C_N 0.62 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.27 Possibly duplicate

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

Overview

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LISC-III 3613 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close^* distance, below the mid-plane, affected by low extinction. It is catalogued as a metal-poor cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~0.39 kpc) differs significantly from the median photometric distance (~0.19 kpc).

Very close Low extinction Metal-poor

Data

🔍 Search references for LISC-III 3613 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	–	77.171	-3.083	2.591	1.216	-0.803	24.098
Chi et al.	2023	77.371	-3.062	2.636	1.126	-0.804	–

💡 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
Chi et al.	2023	0.19	0.50	–	–	-0.642	–	0.54	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 59	73.0	77.14	-3.21	2.58	1.21	-0.94	22.68	0.51

💡 Note: The % column shows the percentage of members that LISC-III 3613 shares with each listed object.

Visualization

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