FSR 1151

(MWSC 935)

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 CC

Number of members (P>50%) 20

Radius (P>50% members) 5.5 [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 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FSR 1151 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, 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 (~3.87 kpc) differs significantly from the median photometric distance (~2.86 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 1151 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	–	99.305	-10.057	0.259	-0.547	-0.216	–
Just et al.	2023	99.286	-10.083	–	–	–	–
Bica et al.	2019	99.304	-10.081	–	–	–	–
Kharchenko et al.	2016	99.286	-10.083	–	–	–	–
Kharchenko et al.	2013	99.292	-10.085	–	1.6	1.09	–
Froebrich et al.	2007	99.304	-10.082	–	–	–	–

💡 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	–	–	–	776	–	269	–	–
Kharchenko et al.	2016	2.86	3.03	–	776	–	–	–	–
Kharchenko et al.	2013	2.86	3.03	–	776	–	–	–	–

Visualization

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