FSR 1447

(MWSC 1445)

0.18 UTI

0.0

C_N

0.16

C_dens

0.25

C_C3

0.25

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 20

Radius (P>50% members) 6.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.16 Very loose
C_C3 0.25 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

ℹ️

FSR 1447 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as an 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.

Relatively close Moderate extinction Old

Data

🔍 Search references for FSR 1447 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	122.91	-51.014	0.36	-3.718	6.439	–
Just et al.	2023	122.884	-51.018	–	–	–	–
Kharchenko et al.	2016	122.884	-51.018	–	–	–	–
Kharchenko et al.	2013	122.887	-51.02	–	-3.0	2.85	–
Froebrich et al.	2007	122.883	-51.024	–	–	–	–

💡 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	–	62	–	–
Kharchenko et al.	2016	2.55	2.58	–	1259	–	–	–	–
Kharchenko et al.	2013	2.55	2.58	–	1259	–	–	–	–

Visualization

ℹ️