FoF 386

0.06 UTI

0.39

C_N

0.7

C_dens

1.0

C_C3

0.0

C_lit

0.15

C_dup

N₅₀ (P>50% members) 39

Stellar density (N₅₀/rad) 3.5 [N/pc²]

C3 classification AA

C_N 0.39 Poorly populated
C_dens 0.7 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.15 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

FoF 386 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

⚠️ Warning: This is 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 Intermediate age

Data

🔍 Search references for FoF 386 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	122.85	-31.956	0.244	-2.601	3.122	58.396
Liu & Pang	2019	122.871	-32.049	0.255	-2.534	3.076	–

💡 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–	–	–	–	576	0.250	–	–	–
Liu & Pang	2019	–	–	–	576	0.250	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Ruprecht 54	84.6	122.84	-31.95	0.22	-2.66	3.16	58.4	0.91

💡 Note: The % column shows the percentage of members that FoF 386 shares with each listed object.

Visualization

ℹ️