FoF 2178

0.23 UTI

0.44

C_N

0.87

C_dens

0.75

C_C3

0.0

C_lit

0.57

C_dup

N₅₀ (P>50% members) 44

Stellar density (N₅₀/rad) 4.3 [N/pc²]

C3 classification AB

C_N 0.44 Poorly populated
C_dens 0.87 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.57 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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FoF 2178 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a metal-rich, very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

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

Metal-rich Very young

Data

🔍 Search references for FoF 2178 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–	303.581	36.707	0.483	-2.881	-5.697	3.457
Liu & Pang	2019	303.573	36.71	0.48	-2.881	-5.695	–

💡 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–	–	–	–	13	0.500	–	–	–
Liu & Pang	2019	–	–	–	13	0.500	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 369	100.0	303.58	36.7	0.48	-2.9	-5.7	-0.68	0.19
Dolidze 3	43.2	303.82	36.83	0.49	-2.87	-5.63	-26.2	0.87

💡 Note: The % column shows the percentage of members that FoF 2178 shares with each listed object.

Visualization

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