FSR 1732

(MWSC 2485)

0.28 UTI

0.0

C_N

0.02

C_dens

0.5

C_C3

0.44

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 12

Radius (P>50% members) 4.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.44 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 1732 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by high extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~7.87 kpc) differs significantly from the median photometric distance (~3.58 kpc).

Distant High extinction Old

Data

🔍 Search references for FSR 1732 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	–	253.72	-49.307	0.127	-4.979	-4.789	-62.967
Just et al.	2023	253.767	-49.325	–	–	–	–
Bica et al.	2019	253.769	-49.328	–	–	–	–
Kharchenko et al.	2016	253.767	-49.325	–	–	–	–
Dias et al.	2014	253.771	-49.326	–	1.23	-2.86	–
Kharchenko et al.	2013	253.777	-49.325	–	0.92	-2.86	–
Froebrich et al.	2007	253.771	-49.326	–	–	–	–
Dias et al.	2002	253.771	-49.326	–	0.92	-2.86	–

💡 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	–	–	–	1995	–	804	–	–
Kharchenko et al.	2016	3.58	3.16	–	1995	–	–	–	–
Kharchenko et al.	2013	3.58	3.16	–	1995	–	–	–	–
Dias et al.	2002	3.58	3.16	–	1995	–	–	–	–

Visualization

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