FSR 0089

(MWSC 2997)

0.39 UTI

0.0

C_N

1.0

C_dens

0.25

C_C3

0.35

C_lit

1.0

C_dup

N₅₀ (P>50% members) 20

Stellar density (N₅₀/rad) 17.0 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.25 Low quality
C_lit 0.35 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FSR 0089 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by very high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.48 kpc) differs significantly from the median photometric distance (~1.52 kpc).

Relatively close Very high extinction Intermediate age

Data

🔍 Search references for FSR 0089 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	99999–	282.154	-3.523	0.403	-2.917	-4.873	–
Just et al.	2023	282.176	-3.52	–	–	–	–
Bica et al.	2019	282.162	-3.51	–	–	–	–
Kharchenko et al.	2016	282.176	-3.52	–	–	–	–
Kharchenko et al.	2013	282.183	-3.519	–	-1.09	-2.82	–
Froebrich et al.	2007	282.163	-3.509	–	–	–	–
Dias et al.	2002	282.163	-3.509	–	1.03	-2.91	–

💡 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]	B_frac	BSS
UCC	99999–	1.52	5.74	–	200	–	71	–	–
Just et al.	2023	–	–	–	200	–	71	–	–
Kharchenko et al.	2016	1.52	5.74	–	200	–	–	–	–
Kharchenko et al.	2013	1.52	5.74	–	200	–	–	–	–
Dias et al.	2002	1.52	5.74	–	200	–	–	–	–

Visualization

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