LISC-III 1182

0.03 UTI

0.0

C_N

0.02

C_dens

0.12

C_C3

0.0

C_lit

0.96

C_dup

C3 classification DC

Number of members (P>50%) 18

Radius (P>50% members) 11.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.96 Unique

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

Overview

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LISC-III 1182 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Low extinction Near-solar metallicity

Data

🔍 Search references for LISC-III 1182 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	–	106.019	20.662	0.267	-0.25	-1.404	16.508
Chi et al.	2023	106.059	20.657	0.294	-0.225	-1.434	–

💡 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	4.37	0.38	–	–	0.274	–	0.46	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Zeta Gemini	4.0	105.97	20.56	0.27	-0.74	-1.59	39.17	0.09

💡 Note: The % column shows the percentage of members that LISC-III 1182 shares with each listed object.

Visualization

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