FSR 1132

(MWSC 742)

0.17 UTI

0.0

C_N

0.09

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) 5.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.09 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 1132 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 high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.69 kpc) differs significantly from the median photometric distance (~1.89 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.

Relatively close High extinction Intermediate age

Data

🔍 Search references for FSR 1132 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	92.066	-11.48	0.213	-0.626	0.258	–
Just et al.	2023	92.079	-11.499	–	–	–	–
Kharchenko et al.	2016	92.079	-11.499	–	–	–	–
Kharchenko et al.	2013	92.085	-11.5	–	4.54	0.48	–
Froebrich et al.	2007	92.108	-11.511	–	–	–	–

💡 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	–	–	–	708	–	156	–	–
Kharchenko et al.	2016	1.89	3.03	–	708	–	–	–	–
Kharchenko et al.	2013	1.89	3.03	–	708	–	–	–	–

Visualization

ℹ️