FoF 2387

0.52 UTI

1.0

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.87

C_dup

C3 classification AA

Number of members (P>50%) 700

Radius (P>50% members) 53.0 [arcmin]

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 0.87 Very likely unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FoF 2387 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, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

Note: This is very likely a unique object, which shares a small 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 2387 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	–	117.394	-46.67	2.531	-4.71	8.959	17.631
He et al.	2022	117.449	-46.862	2.523	-4.759	8.906	–

💡 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]	Bfr	BSS
He et al.	2022	–	0.30	–	11	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 200	88.1	117.36	-46.54	2.54	-4.69	9.01	17.63	0.04
OC 0470	12.9	117.34	-46.37	2.55	-4.71	9.06	17.63	0.66
CWWL 3526	7.1	117.91	-46.81	2.54	-4.78	8.82	19.74	0.0
CWWDL 14576	3.6	116.76	-47.37	2.52	-4.68	8.88	20.47	0.0
OC 0468	3.6	117.31	-46.26	2.57	-4.73	9.26	16.68	0.4
OCSN 199	0.1	119.78	-49.16	2.47	-5.39	8.25	20.01	0.43

💡 Note: The % column shows the percentage of members that FoF 2387 shares with each listed object.

Visualization

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