FSR 0190

(MWSC 3250)

0.21 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.44

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 12

Radius (P>50% members) 6.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.12 Very low quality
C_lit 0.44 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 0190 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.

Distant Moderate extinction Very young

Data

🔍 Search references for FSR 0190 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	–	301.377	33.552	0.22	-3.237	-5.169	-11.402
Just et al.	2023	301.367	33.564	–	–	–	–
Bica et al.	2019	301.38	33.569	–	–	–	–
Kharchenko et al.	2016	301.367	33.564	–	–	–	–
Dias et al.	2014	301.367	33.575	–	-2.73	-6.95	–
Kharchenko et al.	2013	301.372	33.567	–	-3.62	-2.24	–
Froebrich et al.	2007	301.367	33.575	–	–	–	–
Dias et al.	2002	301.367	33.575	–	-2.73	-6.95	–

💡 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	–	–	–	1	–	136	–	–
Kharchenko et al.	2016	3.92	2.71	–	1	–	–	–	–
Kharchenko et al.	2013	3.92	2.71	–	1	–	–	–	–
Dias et al.	2002	3.92	2.71	–	1	–	–	–	–

Visualization

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