FoF 1332

(LP 1332)

0.09 UTI

0.0

C_N

0.09

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 18

Radius (P>50% members) 7.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.09 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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FoF 1332 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Massive Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.

Data

🔍 Search references for FoF 1332 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	–	26.929	60.44	0.34	-1.015	-0.471	–
Almeida et al.	2025	26.851	60.513	–	–	–	–
Dias et al.	2021	26.851	60.513	0.316	-1.015	-0.435	-56.742
Liu & Pang	2019	26.94	60.422	0.321	-0.979	-0.494	–

💡 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
Almeida et al.	2025	2.70	1.78	–	59	–	2631	–	–
Dias et al.	2021	2.70	1.78	–	59	0.051	–	–	–
Liu & Pang	2019	–	–	–	191	0.500	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 4108	20.0	26.73	60.44	0.36	-1.04	-0.58	–	0.13

💡 Note: The % column shows the percentage of members that FoF 1332 shares with each listed object.

Visualization

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