FSR 0333

(MWSC 3562)

0.66 UTI

0.54

C_N

1.0

C_dens

0.75

C_C3

0.5

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 58

Radius (P>50% members) 1.6 [arcmin]

C_N 0.54 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

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

Overview

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FSR 0333 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a very massive, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

Very distant High extinction Very massive Intermediate age

Data

🔍 Search references for FSR 0333 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	–	326.791	54.925	0.155	-1.648	-1.57	-47.489
He et al.	2023	326.792	54.925	0.168	-1.641	-1.584	-47.49
Just et al.	2023	326.785	54.924	–	–	–	–
Bica et al.	2019	326.793	54.937	–	–	–	–
Kharchenko et al.	2016	326.785	54.924	–	–	–	–
Kharchenko et al.	2013	326.79	54.928	–	-3.3	-1.4	–
Kharchenko et al.	2012	326.79	54.928	–	-3.3	-1.4	–
Froebrich et al.	2007	326.788	54.939	–	–	–	–
Dias et al.	2002	326.788	54.939	–	-1.15	-2.72	–

💡 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
He et al.	2023	4.17	3.80	–	794	–	–	–	–
Just et al.	2023	–	–	–	785	–	6501	–	–
Kharchenko et al.	2016	6.00	3.41	–	785	–	–	–	–
Kharchenko et al.	2013	6.00	3.41	–	785	–	–	–	–
Kharchenko et al.	2012	6.00	3.41	–	785	–	–	–	–
Dias et al.	2002	6.00	3.41	–	785	–	–	–	–

Visualization

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