FSR 0522

(MWSC 89)

0.66 UTI

0.48

C_N

1.0

C_dens

0.5

C_C3

0.65

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 48

Radius (P>50% members) 1.7 [arcmin]

C_N 0.48 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.65 Moderately studied
C_dup 1.0 Unique

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

Overview

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FSR 0522 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the distance and age parameters (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~6.01 kpc) differs significantly from the median photometric distance (~2.09 kpc).

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for FSR 0522 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	–	13.443	65.794	0.167	-1.588	-0.47	-19.143
Hunt & Reffert	2024	13.378	65.795	0.159	-1.593	-0.46	-19.188
Cavallo et al.	2024	13.417	65.786	0.16	–	–	–
He et al.	2023	13.442	65.796	0.167	-1.624	-0.443	–
Hunt & Reffert	2023	13.378	65.795	0.159	-1.593	-0.46	-19.188
Just et al.	2023	13.488	65.793	–	–	–	–
Kharchenko et al.	2016	13.488	65.793	–	–	–	–
Dias et al.	2014	13.458	65.793	–	-5.49	-2.34	–
Kharchenko et al.	2013	13.5	65.797	–	-1.16	1.93	–
Kharchenko et al.	2012	13.5	65.797	–	-0.7	1.18	–
Froebrich et al.	2007	13.458	65.793	–	–	–	–
Dias et al.	2002	13.458	65.793	–	-0.7	1.18	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	942*	–	–
Cavallo et al.	2024	2.83	3.83	–	81	0.120	–	–	–
He et al.	2023	10.96	5.10	–	3	–	–	–	–
Hunt & Reffert	2023	6.19	4.21	1.52	10	–	–	–	–
Just et al.	2023	–	–	–	355	–	40	–	–
Kharchenko et al.	2016	2.09	2.84	–	355	–	–	–	–
Kharchenko et al.	2013	2.09	2.84	–	355	–	–	–	–
Kharchenko et al.	2012	1.51	2.71	–	1189	–	–	–	–
Dias et al.	2002	1.51	2.71	–	1189	–	–	–	–

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

Visualization

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