FoF 1487

(LP 1487)

0.47 UTI

0.64

C_N

0.96

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 77

Radius (P>50% members) 4.3 [arcmin]

C_N 0.64 Moderately populated
C_dens 0.96 Very dense
C_C3 0.75 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 1487 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

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

Relatively close Moderate extinction Massive Near-solar metallicity Very young

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

Data

🔍 Search references for FoF 1487 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	–	160.501	-58.386	0.313	-6.527	3.414	4.268
Almeida et al.	2025	160.492	-58.373	–	–	–	–
Dias et al.	2021	160.492	-58.373	0.314	-6.611	3.24	–

💡 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	2.83	1.84	–	13	–	1004	–	–
Dias et al.	2021	2.83	1.84	–	13	-0.004	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 2554	72.7	160.45	-58.38	0.32	-6.49	3.45	-10.0	0.31

💡 Note: The % column shows the percentage of members that FoF 1487 shares with each listed object.

Visualization

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