FSR 0067

(MWSC 3055)

0.20 UTI

0.0

C_N

0.1

C_dens

0.25

C_C3

0.31

C_lit

1.0

C_dup

C3 classification DB

Number of members (P>50%) 15

Radius (P>50% members) 6.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.1 Very loose
C_C3 0.25 Low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

FSR 0067 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a very massive, old cluster (see Parameters). It is poorly 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.

Distant Moderate extinction Very massive Old

Data

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	287.416	-13.922	0.32	-2.974	-6.329	–
Just et al.	2023	287.4	-13.902	–	–	–	–
Bica et al.	2019	287.384	-13.888	–	–	–	–
Kharchenko et al.	2016	287.4	-13.902	–	–	–	–
Kharchenko et al.	2013	287.407	-13.9	–	0.28	-8.37	–
Froebrich et al.	2007	287.379	-13.892	–	–	–	–

💡 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	–	–	–	1259	–	6934	–	–
Kharchenko et al.	2016	4.08	1.42	–	1259	–	–	–	–
Kharchenko et al.	2013	4.08	1.42	–	1259	–	–	–	–

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.

Visualization

💡 Note: How are the galactocentric plots generated? See FAQ.