FSR 1191

(MWSC 1005)

0.20 UTI

0.0

C_N

0.01

C_dens

0.38

C_C3

0.31

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 8

Radius (P>50% members) 5.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.38 Low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

ℹ️

FSR 1191 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* 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 (~8.14 kpc) differs significantly from the median photometric distance (~3.36 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.

Distant Moderate extinction Old

Data

🔍 Search references for FSR 1191 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	103.109	-13.229	0.123	-0.488	0.745	87.708
Just et al.	2023	103.114	-13.233	–	–	–	–
Bica et al.	2019	103.126	-13.234	–	–	–	–
Kharchenko et al.	2016	103.114	-13.233	–	–	–	–
Kharchenko et al.	2013	103.12	-13.235	–	0.9	0.33	–
Froebrich et al.	2007	103.121	-13.235	–	–	–	–

💡 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	–	597	–	–
Kharchenko et al.	2016	3.36	1.62	–	1259	–	–	–	–
Kharchenko et al.	2013	3.36	1.62	–	1259	–	–	–	–

Visualization

ℹ️