FoF 2435

0.00 UTI

0.79

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 204

Radius (P>50% members) 32.9 [arcmin]

C_N 0.79 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 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FoF 2435 is a 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.

⚠️ 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.

Low extinction Very young

Data

🔍 Search references for FoF 2435 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	–	167.163	-77.196	5.246	-22.533	0.282	13.924
He et al.	2022	167.293	-77.044	5.247	-22.508	0.303	–

💡 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	–	0.65	–	4	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Chamaleon I	100.0	167.16	-77.2	5.25	-22.53	0.29	13.92	0.71
OCSN 188	48.0	167.09	-77.49	5.29	-23.05	0.59	14.59	0.0
CWWDL 14679	41.2	167.44	-76.55	5.2	-22.07	-0.25	14.71	0.0
OC 0579	29.9	167.09	-77.56	5.27	-23.03	0.59	17.54	0.0
OCSN 187	27.5	167.49	-76.53	5.2	-21.84	-0.45	12.25	0.0
OC 0578	24.5	167.51	-76.51	5.19	-21.83	-0.52	12.25	0.0

💡 Note: The % column shows the percentage of members that FoF 2435 shares with each listed object.

Visualization

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