FSR 1574

(MWSC 1972)

0.21 UTI

0.26

C_N

0.16

C_dens

0.12

C_C3

0.25

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 26

Radius (P>50% members) 7.1 [arcmin]

C_N 0.26 Poorly populated
C_dens 0.16 Very loose
C_C3 0.12 Very 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

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FSR 1574 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, well above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.76 kpc) differs significantly from the median photometric distance (~1.39 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 Low extinction Old

Data

🔍 Search references for FSR 1574 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	–	176.201	-45.68	0.363	-10.792	1.118	7.925
Just et al.	2023	176.167	-45.657	–	–	–	–
Kharchenko et al.	2016	176.167	-45.657	–	–	–	–
Kharchenko et al.	2013	176.175	-45.66	–	-6.48	-0.53	–
Froebrich et al.	2007	176.183	-45.663	–	–	–	–

💡 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	–	–	–	1778	–	185	–	–
Kharchenko et al.	2016	1.39	0.84	–	1778	–	–	–	–
Kharchenko et al.	2013	1.39	0.84	–	1778	–	–	–	–

Visualization

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