FSR 0477

(MWSC 36)

0.20 UTI

0.0

C_N

0.12

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 22

Radius (P>50% members) 5.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.12 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 0477 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.76 kpc) differs significantly from the median photometric distance (~1.91 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 Old

Data

🔍 Search references for FSR 0477 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	–	5.815	51.858	0.266	-2.74	-2.15	–
Just et al.	2023	5.736	51.879	–	–	–	–
Bica et al.	2019	5.764	51.876	–	–	–	–
Kharchenko et al.	2016	5.736	51.879	–	–	–	–
Kharchenko et al.	2013	5.745	51.883	–	-3.76	2.02	–
Kharchenko et al.	2012	5.745	51.883	–	-3.76	2.02	–
Froebrich et al.	2007	5.758	51.879	–	–	–	–

💡 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	–	–	–	1096	–	107	–	–
Kharchenko et al.	2016	1.91	1.42	–	1096	–	–	–	–
Kharchenko et al.	2013	1.91	1.42	–	1096	–	–	–	–
Kharchenko et al.	2012	1.91	1.42	–	1096	–	–	–	–

Visualization

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