FSR 0034

(MWSC 3031)

0.15 UTI

0.0

C_N

0.02

C_dens

0.12

C_C3

0.31

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 13

Radius (P>50% members) 6.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.12 Very low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 0034 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, well below the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~7.12 kpc) differs significantly from the median photometric distance (~1.88 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Young

Data

🔍 Search references for FSR 0034 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	–	284.75	-26.82	0.14	-4.435	-5.102	50.728
Just et al.	2023	284.675	-26.795	–	–	–	–
Bica et al.	2019	284.689	-26.791	–	–	–	–
Kharchenko et al.	2016	284.675	-26.795	–	–	–	–
Kharchenko et al.	2013	284.683	-26.794	–	1.77	-10.37	–
Froebrich et al.	2007	284.683	-26.794	–	–	–	–

💡 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
Just et al.	2023	–	–	–	32	–	217	–	–
Kharchenko et al.	2016	1.88	3.23	–	32	–	–	–	–
Kharchenko et al.	2013	1.88	3.23	–	32	–	–	–	–

Visualization

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