FoF 676

(LP 0676)

0.54 UTI

0.72

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 94

Radius (P>50% members) 2.8 [arcmin]

C_N 0.72 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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FoF 676 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 3 later reported entries. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Old

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.

Data

🔍 Search references for FoF 676 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	–	149.033	-60.182	0.332	-5.877	5.221	-0.082
Almeida et al.	2025	149.023	-60.176	–	–	–	–
Dias et al.	2021	149.023	-60.176	0.295	-5.871	5.184	-0.555

💡 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
Almeida et al.	2025	2.41	0.66	–	3281	–	418	–	–
Dias et al.	2021	2.41	0.66	–	3281	-0.039	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 6242	95.7	149.03	-60.18	0.33	-5.87	5.22	0.66	0.04
OC 0534	91.5	149.03	-60.18	0.33	-5.88	5.22	0.81	0.02
CWWDL 214	43.6	149.03	-60.18	0.33	-5.89	5.21	1.81	0.0

💡 Note: The % column shows the percentage of members that FoF 676 shares with each listed object.

Visualization

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