LISC-III 3611

0.17 UTI

0.45

C_N

0.34

C_dens

0.5

C_C3

0.0

C_lit

0.67

C_dup

C3 classification BB

Number of members (P>50%) 45

Radius (P>50% members) 44.6 [arcmin]

C_N 0.45 Poorly populated
C_dens 0.34 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.67 Likely unique

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

Overview

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LISC-III 3611 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a very close^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~0.39 kpc) differs significantly from the median photometric distance (~0.63 kpc).

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.

Close Moderate extinction Metal-poor

Data

🔍 Search references for LISC-III 3611 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	–	76.327	9.026	2.535	0.811	-4.535	15.563
Chi et al.	2023	76.182	8.973	2.54	0.891	-4.546	–

💡 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	0.63	1.50	–	–	-0.642	–	0.55	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 522	33.3	75.97	8.08	2.57	0.98	-4.46	17.92	0.36

💡 Note: The % column shows the percentage of members that LISC-III 3611 shares with each listed object.

Visualization

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