FSR 0628

(MWSC 272)

0.15 UTI

0.0

C_N

0.04

C_dens

0.25

C_C3

0.23

C_lit

1.0

C_dup

N_m (P>50%) 22

Core radius and density 2.2 [pc], 0.2 [pc^-2]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.25 Low quality
C_lit 0.23 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FSR 0628 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature.

⚠️ 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.

Very distant High extinction Old

Data

🔍 Search references for FSR 0628 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	99999–	50.779	60.577	0.232	-0.752	0.016	–
Just et al.	2023	50.788	60.548	–	–	–	–
Bica et al.	2019	50.809	60.56	–	–	–	–
Sampedro et al.	2017	50.8	60.563	–	-1.55	-4.42	–
Kharchenko et al.	2016	50.788	60.548	–	–	–	–
Dias et al.	2014	50.8	60.563	–	-1.55	-1.34	–
Kharchenko et al.	2013	50.8	60.55	–	-1.42	-4.38	–
Kharchenko et al.	2012	50.8	60.55	–	-1.42	-4.38	–
Froebrich et al.	2007	50.8	60.563	–	–	–	–
Dias et al.	2002	50.8	60.563	–	-1.55	-1.34	–

💡 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]	B_frac	BSS
UCC	99999–	5.0	3.31	–	1778	–	188	–	–
Just et al.	2023	–	–	–	1778	–	188	–	–
Kharchenko et al.	2016	5.00	3.31	–	1778	–	–	–	–
Kharchenko et al.	2013	5.00	3.31	–	1778	–	–	–	–
Kharchenko et al.	2012	5.00	3.31	–	1778	–	–	–	–
Dias et al.	2002	5.00	3.31	–	1778	–	–	–	–

Visualization

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