FSR 0148

(MWSC 3145)

0.20 UTI

0.0

C_N

0.04

C_dens

0.38

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 16

Stellar density (N₅₀/rad) 0.2 [N/pc²]

C3 classification BC

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.38 Low quality
C_lit 0.3 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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FSR 0148 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by very high extinction. It is catalogued as a low-mass, very young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.97 kpc) differs significantly from the median photometric distance (~0.94 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.

Close Very high extinction Low mass Very young

Data

🔍 Search references for FSR 0148 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–	294.36	21.265	0.252	-3.145	-6.168	–
Just et al.	2023	294.361	21.312	–	–	–	–
Bica et al.	2019	294.368	21.318	–	–	–	–
Kharchenko et al.	2016	294.361	21.312	–	–	–	–
Kharchenko et al.	2013	294.367	21.315	–	-4.07	-11.18	–
Froebrich et al.	2007	294.367	21.314	–	–	–	–

💡 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–	0.94	5.13	–	1	–	19	–	–
Just et al.	2023	–	–	–	1	–	19	–	–
Kharchenko et al.	2016	0.94	5.13	–	1	–	–	–	–
Kharchenko et al.	2013	0.94	5.13	–	1	–	–	–	–

Visualization

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