FoF 2295

0.49 UTI

0.79

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.88

C_dup

C3 classification AA

Number of members (P>50%) 218

Radius (P>50% members) 17.7 [arcmin]

C_N 0.79 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.88 Very likely unique

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

Overview

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FoF 2295 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

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

Relatively close Low extinction Metal-rich Intermediate age

Data

🔍 Search references for FoF 2295 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	–	333.046	53.919	0.914	-1.783	-2.346	-25.143
Wei et al.	2025	333.105	53.955	0.921	-1.775	-2.346	–
He et al.	2022	333.091	53.963	0.915	-1.774	-2.354	–

💡 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	1.35	0.66	–	501	0.500	365	0.52	–
He et al.	2022	–	1.05	–	141	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14131	84.4	333.06	53.92	0.92	-1.78	-2.35	-25.59	0.0
OC 0165	11.5	333.01	53.9	0.91	-1.77	-2.38	-25.59	0.33

💡 Note: The % column shows the percentage of members that FoF 2295 shares with each listed object.

Visualization

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