FoF 1614

(LP 1614)

0.55 UTI

0.77

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%) 145

Radius (P>50% members) 3.1 [arcmin]

C_N 0.77 Rich
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 1614 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Near-solar metallicity Very young

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

Data

🔍 Search references for FoF 1614 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	–	241.566	-52.134	0.365	-2.849	-4.802	-34.475
Almeida et al.	2025	241.562	-52.142	–	–	–	–
Almeida et al.	2023	241.561	-52.141	–	–	–	–
Dias et al.	2021	241.562	-52.142	0.359	-2.837	-4.769	–

💡 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	2.48	3.28	–	12	–	854	–	–
Almeida et al.	2023	2.12	3.28	–	64	0.152	818*	0.72	–
Dias et al.	2021	2.48	3.28	–	12	0.165	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0644	17.2	241.56	-52.14	0.37	-2.86	-4.82	-36.03	0.0

💡 Note: The % column shows the percentage of members that FoF 1614 shares with each listed object.

Visualization

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