FoF 2442

0.00 UTI

1.0

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 587

Stellar density (N₅₀/rad) 57.0 [N/pc²]

C3 classification AA

C_N 1.0 Very 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 2442 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane. It is catalogued as a near-solar metallicity, very 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 Very young

Data

🔍 Search references for FoF 2442 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–	250.216	-39.534	5.673	-11.919	-21.297	0.21
Liu & Pang	2019	250.372	-39.565	5.658	-11.894	-21.208	–

💡 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–	–	–	–	6	0.000	–	–	–
Liu & Pang	2019	–	–	–	6	0.000	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 640	100.0	250.2	-39.53	5.68	-11.94	-21.35	0.54	0.9
OCSN 212	95.7	250.14	-39.52	5.68	-11.94	-21.32	0.2	0.0
CWNU 1146	1.2	252.86	-38.13	6.03	-11.84	-22.52	-4.5	0.0

💡 Note: The % column shows the percentage of members that FoF 2442 shares with each listed object.

Visualization

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