FSR 0317

(MWSC 3525; Kernya 8)

0.25 UTI

0.0

C_N

0.11

C_dens

0.12

C_C3

0.5

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 20

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

C_N 0.0 Sparse
C_dens 0.11 Very loose
C_C3 0.12 Very low quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

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

Overview

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FSR 0317 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~3.99 kpc) differs significantly from the median photometric distance (~1.93 kpc).

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for FSR 0317 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	–	323.236	53.704	0.251	-3.69	-2.534	–
Just et al.	2023	323.149	53.751	–	–	–	–
Bica et al.	2019	323.151	53.763	–	–	–	–
Kharchenko et al.	2016	323.149	53.751	–	–	–	–
Dias et al.	2014	323.154	53.763	–	0.35	-0.54	–
Kharchenko et al.	2013	323.154	53.755	–	-3.21	0.08	–
Kharchenko et al.	2012	323.154	53.755	–	-3.21	0.08	–
Froebrich et al.	2007	323.154	53.763	–	–	–	–
Dias et al.	2002	323.154	53.763	–	-3.21	0.08	–

💡 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	–	50	–	–
Kharchenko et al.	2016	1.93	2.58	–	631	–	–	–	–
Kharchenko et al.	2013	1.93	2.58	–	631	–	–	–	–
Kharchenko et al.	2012	1.93	2.58	–	631	–	–	–	–
Dias et al.	2002	1.93	2.58	–	631	–	–	–	–

Visualization

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