FSR 0210

(MWSC 3340)

0.24 UTI

0.0

C_N

0.21

C_dens

0.12

C_C3

0.44

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 19

Radius (P>50% members) 5.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.21 Very loose
C_C3 0.12 Very low quality
C_lit 0.44 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 0210 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.61 kpc) differs significantly from the median photometric distance (~1.09 kpc).

Relatively close Moderate extinction Low mass Intermediate age

Data

🔍 Search references for FSR 0210 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	–	306.583	37.288	0.383	-2.778	-4.3	-6.781
Just et al.	2023	306.632	37.263	–	–	–	–
Bica et al.	2019	306.662	37.28	–	–	–	–
Kharchenko et al.	2016	306.632	37.263	–	–	–	–
Dias et al.	2014	306.654	37.281	–	1.46	-0.33	–
Kharchenko et al.	2013	306.637	37.266	–	2.92	-0.74	–
Froebrich et al.	2007	306.654	37.281	–	–	–	–
Dias et al.	2002	306.654	37.281	–	1.46	-0.33	–

💡 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
Just et al.	2023	–	–	–	631	–	13	–	–
Kharchenko et al.	2016	1.09	2.58	–	631	–	–	–	–
Kharchenko et al.	2013	1.09	2.58	–	631	–	–	–	–
Dias et al.	2002	1.09	2.58	–	631	–	–	–	–

Visualization

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