FSR 1432

(SAI 97; MWSC 1594)

0.40 UTI

0.0

C_N

1.0

C_dens

0.38

C_C3

0.31

C_lit

1.0

C_dup

C3 classification CB

Number of members (P>50%) 23

Radius (P>50% members) 2.8 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
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

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FSR 1432 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by high extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.48 kpc) differs significantly from the median photometric distance (~1.90 kpc).

Relatively close High extinction Low mass Intermediate age

Data

🔍 Search references for FSR 1432 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	–	133.224	-44.206	0.403	-5.185	4.157	–
Just et al.	2023	133.228	-44.182	–	–	–	–
Kharchenko et al.	2016	133.228	-44.182	–	–	–	–
Kharchenko et al.	2013	133.233	-44.185	–	-4.94	6.18	–
Glushkova et al.	2010	133.222	-44.202	–	–	–	–
Froebrich et al.	2007	133.229	-44.211	–	–	–	–

💡 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	–	–	–	126	–	41	–	–
Kharchenko et al.	2016	1.90	3.87	–	126	–	–	–	–
Kharchenko et al.	2013	1.90	3.87	–	126	–	–	–	–

Visualization

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