FoF 2275

0.00 UTI

0.76

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%) 134

Radius (P>50% members) 12.4 [arcmin]

C_N 0.76 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 2275 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

⚠️ 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.

Near-solar metallicity Young

Data

🔍 Search references for FoF 2275 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	–	346.45	49.381	1.797	2.634	-1.946	-11.112
Liu & Pang	2019	346.45	49.41	1.794	2.652	-1.909	–

💡 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
Liu & Pang	2019	–	–	–	32	0.250	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 171	100.0	346.41	49.38	1.79	2.64	-1.99	-11.02	0.08
UPK 185	100.0	346.41	49.38	1.79	2.64	-1.96	-11.02	0.86
CWWDL 14300	37.3	346.43	49.39	1.81	2.62	-1.93	-10.54	0.0

💡 Note: The % column shows the percentage of members that FoF 2275 shares with each listed object.

Visualization

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