FoF 2236

(LP 2236)

0.00 UTI

0.79

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 201

Stellar density (N₅₀/rad) 25.7 [N/pc²]

C3 classification AA

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 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FoF 2236 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 near-solar metallicity, old 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.

Note: This object contains blue stragglers according to at least one source.

Relatively close Low extinction Near-solar metallicity Old Contains BSS

Data

🔍 Search references for FoF 2236 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	99999–	146.461	-52.489	0.977	-1.652	-0.41	-4.431
Li et al.	2023	146.494	-52.489	0.97	-1.64	-0.43	–
Liu & Pang	2019	146.428	-52.493	0.959	-1.661	-0.441	–

💡 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]	B_frac	BSS
UCC	99999–	1.26	0.85	–	1912	-0.264	–	–	1
Li et al.	2023	1.26	0.85	–	1585	0.223	–	–	1⁽¹⁾
Liu & Pang	2019	–	–	–	2240	-0.750	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 256	100.0	146.46	-52.49	0.98	-1.65	-0.41	-4.5	0.02
UPK 549	99.5	146.46	-52.49	0.98	-1.65	-0.41	-4.5	0.74

💡 Note: The % column shows the percentage of members that FoF 2236 shares with each listed object.

Visualization

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