FSR 1129

(MWSC 1042)

0.53 UTI

0.28

C_N

1.0

C_dens

0.5

C_C3

0.44

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 28

Radius (P>50% members) 5.2 [arcmin]

C_N 0.28 Poorly populated
C_dens 1.0 Very dense
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 1129 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for FSR 1129 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	–	104.69	-4.867	0.719	-0.475	0.294	11.233
Hunt & Reffert	2024	104.712	-4.853	0.713	-0.449	0.285	11.215
Cavallo et al.	2024	104.66	-4.843	0.716	–	–	–
Hunt & Reffert	2023	104.712	-4.853	0.713	-0.449	0.285	11.215
Just et al.	2023	104.686	-4.928	–	–	–	–
Kharchenko et al.	2016	104.686	-4.928	–	–	–	–
Kharchenko et al.	2013	104.692	-4.93	–	-0.11	1.31	–
Froebrich et al.	2007	104.688	-4.935	–	–	–	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	92*	–	–
Cavallo et al.	2024	1.37	0.54	–	115	-0.360	–	–	–
Hunt & Reffert	2023	1.33	0.36	0.49	79	–	–	–	–
Just et al.	2023	–	–	–	243	–	61	–	–
Kharchenko et al.	2016	1.88	2.19	–	243	–	–	–	–
Kharchenko et al.	2013	1.88	2.19	–	243	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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