FSR 0022

(MWSC 2751)

0.26 UTI

0.0

C_N

0.03

C_dens

0.25

C_C3

0.5

C_lit

1.0

C_dup

N_m (P>50%) 18

Core radius and density 3.9 [pc], 0.2 [pc^-2]

C3 classification DB

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.25 Low quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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FSR 0022 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by very high extinction. It is catalogued as a very massive, old cluster (see Parameters). It is moderately studied in the literature.

Distant Very high extinction Very massive Old

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

Data

🔍 Search references for FSR 0022 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–	269.114	-23.211	0.172	-0.547	-3.06	18.593
Just et al.	2023	269.099	-23.193	–	–	–	–
Bica et al.	2019	269.122	-23.196	–	–	–	–
Dias et al.	2018	–	–	–	0.75	-2.08	–
Sampedro et al.	2017	269.117	-23.193	–	2.98	-5.46	–
Dias et al.	2016	269.117	-23.193	–	2.24	-3.89	–
Kharchenko et al.	2016	269.099	-23.193	–	–	–	–
Dias et al.	2014	269.117	-23.193	–	2.06	-4.05	–
Kharchenko et al.	2013	269.107	-23.192	–	-1.22	-6.67	–
Morales et al.	2013	269.117	-23.193	–	–	–	–
Froebrich et al.	2007	269.117	-23.193	–	–	–	–

💡 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–	4.34	5.52	–	4467	–	5420	–	–
Just et al.	2023	–	–	–	4467	–	5420	–	–
Dias et al.	2016	4.34	5.52	–	4467	–	–	–	–
Kharchenko et al.	2016	4.34	5.52	–	4467	–	–	–	–
Kharchenko et al.	2013	4.34	5.52	–	4467	–	–	–	–

Visualization

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