FSR 0225

(MWSC 3402)

0.21 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.44

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 17

Radius (P>50% members) 7.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 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 0225 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by very high extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~5.01 kpc) differs significantly from the median photometric distance (~1.15 kpc).

Relatively close Very high extinction Low mass Intermediate age

Data

🔍 Search references for FSR 0225 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	–	310.738	37.818	0.2	-3.61	-4.189	–
Just et al.	2023	310.712	37.852	–	–	–	–
Bica et al.	2019	310.724	37.833	–	–	–	–
Kharchenko et al.	2016	310.712	37.852	–	–	–	–
Dias et al.	2014	310.721	37.829	–	-2.23	-4.19	–
Kharchenko et al.	2013	310.717	37.855	–	-4.24	-2.83	–
Froebrich et al.	2007	310.721	37.829	–	–	–	–
Dias et al.	2002	310.721	37.829	–	-2.23	-4.19	–

💡 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	–	–	–	733	–	26	–	–
Kharchenko et al.	2016	1.15	6.71	–	733	–	–	–	–
Kharchenko et al.	2013	1.15	6.71	–	733	–	–	–	–
Dias et al.	2002	1.15	6.71	–	733	–	–	–	–

Visualization

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