FSR 0826

(SAI 55; MWSC 653)

0.61 UTI

0.46

C_N

0.47

C_dens

0.12

C_C3

1.0

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 46

Radius (P>50% members) 4.4 [arcmin]

C_N 0.46 Poorly populated
C_dens 0.47 Loose
C_C3 0.12 Very low quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

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

Overview

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FSR 0826 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is very well-studied in the literature.

Relatively close Moderate extinction Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for FSR 0826 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	–	85.769	28.969	0.289	-0.466	-1.542	–
Almeida et al.	2025	85.782	29.005	–	–	–	–
Hunt & Reffert	2024	85.726	28.95	0.298	-0.411	-1.465	9.714
Celli et al.	2024	85.765	28.989	–	–	–	–
Cavallo et al.	2024	85.933	29.108	0.297	–	–	–
Hunt & Reffert	2023	85.726	28.95	0.298	-0.411	-1.465	9.714
Just et al.	2023	85.711	28.957	–	–	–	–
Dias et al.	2021	85.782	29.005	0.264	-0.577	-1.572	–
Cantat-Gaudin et al.	2020	85.765	28.989	0.281	-0.535	-1.585	–
Sánchez et al.	2020	85.717	28.941	–	-0.681	-1.557	–
Cantat-Gaudin & Anders	2020	85.765	28.989	0.281	-0.535	-1.585	–
Cantat-Gaudin et al.	2018	85.765	28.989	0.281	-0.535	-1.585	–
Kharchenko et al.	2016	85.711	28.957	–	–	–	–
Dias et al.	2014	85.717	28.941	–	-0.57	-2.67	–
Kharchenko et al.	2013	85.72	28.957	–	2.19	-2.18	–
Kharchenko et al.	2012	85.72	28.957	–	2.19	-2.18	–
Glushkova et al.	2010	85.713	28.945	–	–	–	–
Froebrich et al.	2007	85.717	28.941	–	–	–	–
Dias et al.	2002	85.717	28.941	–	-0.57	-2.67	–

💡 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
Almeida et al.	2025	2.68	2.62	–	51	–	253	–	–
Hunt & Reffert	2024	–	–	–	–	–	283*	–	–
Celli et al.	2024	–	–	–	5	–	229	–	–
Cavallo et al.	2024	3.12	2.45	–	178	0.620	–	–	–
Hunt & Reffert	2023	2.97	2.64	2.60	78	–	–	–	–
Just et al.	2023	–	–	–	20	–	167	–	–
Dias et al.	2021	2.68	2.62	–	51	-0.142	–	–	–
Cantat-Gaudin et al.	2020	4.81	2.78	–	5	–	–	–	–
Cantat-Gaudin & Anders	2020	3.23	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	3.23	–	–	–	–	–	–	–
Kharchenko et al.	2016	2.10	3.56	–	20	–	–	–	–
Kharchenko et al.	2013	2.10	3.56	–	20	–	–	–	–
Kharchenko et al.	2012	2.10	3.56	–	20	–	–	–	–
Dias et al.	2002	2.10	3.38	–	10	–	–	–	–

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

Visualization

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