FSR 0924

(MWSC 776)

0.38 UTI

0.3

C_N

0.14

C_dens

0.75

C_C3

0.35

C_lit

1.0

C_dup

N₅₀ (P>50% members) 30

Stellar density (N₅₀/rad) 0.7 [N/pc²]

C3 classification AB

C_N 0.3 Poorly populated
C_dens 0.14 Very loose
C_C3 0.75 High quality
C_lit 0.35 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FSR 0924 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large^* 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 (~5.73 kpc) differs significantly from the median photometric distance (~1.72 kpc).

Relatively close High extinction Intermediate age

Data

🔍 Search references for FSR 0924 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	99999–	92.617	16.83	0.174	0.247	-0.363	32.474
Just et al.	2023	92.601	16.834	–	–	–	–
Bica et al.	2019	92.608	16.834	–	–	–	–
Kharchenko et al.	2016	92.601	16.834	–	–	–	–
Kharchenko et al.	2013	92.608	16.833	–	-0.63	-6.97	–
Froebrich et al.	2007	92.608	16.837	–	–	–	–
Dias et al.	2002	92.608	16.837	–	-0.63	-6.97	–

💡 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]	B_frac	BSS
UCC	99999–	1.72	3.1	–	741	–	64	–	–
Just et al.	2023	–	–	–	741	–	64	–	–
Kharchenko et al.	2016	1.72	3.10	–	741	–	–	–	–
Kharchenko et al.	2013	1.72	3.10	–	741	–	–	–	–
Dias et al.	2002	1.72	3.10	–	741	–	–	–	–

Visualization

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