FSR 0293

(MWSC 3514)

0.18 UTI

0.0

C_N

0.05

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 14

Radius (P>50% members) 5.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.12 Very low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 0293 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.89 kpc) differs significantly from the median photometric distance (~2.80 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Low mass Old

Data

🔍 Search references for FSR 0293 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	–	322.001	47.128	0.205	-3.221	-3.176	–
Just et al.	2023	321.97	47.146	–	–	–	–
Bica et al.	2019	321.985	47.123	–	–	–	–
Kharchenko et al.	2016	321.97	47.146	–	–	–	–
Kharchenko et al.	2013	321.975	47.15	–	-2.59	-3.45	–
Kharchenko et al.	2012	321.975	47.15	–	-2.59	-3.45	–
Froebrich et al.	2007	321.983	47.118	–	–	–	–

💡 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	–	–	–	1679	–	41	–	–
Kharchenko et al.	2016	2.80	1.24	–	1679	–	–	–	–
Kharchenko et al.	2013	2.80	1.24	–	1679	–	–	–	–
Kharchenko et al.	2012	2.80	1.24	–	1679	–	–	–	–

Visualization

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