FoF 2417

0.00 UTI

0.75

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 110

Radius (P>50% members) 26.3 [arcmin]

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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FoF 2417 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close^* distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very 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 (~0.55 kpc) differs significantly from the median photometric distance (~0.78 kpc).

Close Low extinction Near-solar metallicity Young

Data

🔍 Search references for FoF 2417 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	–	298.323	26.396	1.833	2.322	-2.155	-16.283
Wei et al.	2025	298.383	26.438	1.833	2.338	-2.167	–
Liu & Pang	2019	298.3	26.437	1.829	2.363	-2.123	–

💡 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
Wei et al.	2025	0.78	0.73	–	49	0.250	150	0.17	–
Liu & Pang	2019	–	–	–	60	0.000	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 82	100.0	298.35	26.41	1.84	2.3	-2.15	-17.01	0.87
CWWDL 14618	23.6	298.49	26.21	1.83	2.36	-2.21	-12.48	0.0

💡 Note: The % column shows the percentage of members that FoF 2417 shares with each listed object.

Visualization

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