FoF 2379

0.16 UTI

0.35

C_N

0.3

C_dens

1.0

C_C3

0.0

C_lit

0.49

C_dup

N₅₀ (P>50% members) 35

Stellar density (N₅₀/rad) 1.5 [N/pc²]

C3 classification AA

C_N 0.35 Poorly populated
C_dens 0.3 Loose
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.49 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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FoF 2379 is a poorly populated, loose object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Low extinction Very young

Data

🔍 Search references for FoF 2379 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–	339.633	38.153	1.98	-1.557	-5.796	-21.268
He et al.	2022	339.461	38.159	1.991	-1.537	-5.677	–

💡 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–	–	0.4	–	14	–	–	–	–
He et al.	2022	–	0.40	–	14	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 39	51.4	339.22	37.76	2.04	-1.76	-6.04	-13.08	0.83
CWWDL 14563	45.7	339.57	38.97	2.0	-1.59	-5.35	-22.61	0.35
OCSN 29	37.1	339.15	37.72	2.03	-1.72	-6.19	-13.08	0.02
CWWDL 14543	28.6	339.72	37.29	2.01	-1.55	-6.12	-13.97	0.12

💡 Note: The % column shows the percentage of members that FoF 2379 shares with each listed object.

Visualization

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