FSR 1412

(MWSC 1513)

0.18 UTI

0.0

C_N

0.04

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 14

Radius (P>50% members) 7.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.12 Very low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 1412 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.53 kpc) differs significantly from the median photometric distance (~2.64 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 Very young

Data

🔍 Search references for FSR 1412 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	–	129.315	-44.141	0.283	-3.843	3.626	–
Just et al.	2023	129.314	-44.128	–	–	–	–
Kharchenko et al.	2016	129.314	-44.128	–	–	–	–
Dias et al.	2014	129.287	-44.153	–	-2.7	-0.98	–
Kharchenko et al.	2013	129.319	-44.131	–	-3.83	7.21	24.1
Froebrich et al.	2007	129.287	-44.153	–	–	–	–
Dias et al.	2002	129.287	-44.153	–	-3.83	7.21	–

💡 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	–	–	–	11	–	668	–	–
Kharchenko et al.	2016	2.64	3.74	–	11	–	–	–	–
Kharchenko et al.	2013	2.64	3.74	–	11	–	–	–	–
Dias et al.	2002	2.64	3.74	–	11	–	–	–	–

Visualization

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