FSR 0051

(MWSC 2843)

0.20 UTI

0.0

C_N

0.01

C_dens

0.25

C_C3

0.38

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 16

Radius (P>50% members) 6.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.25 Low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 0051 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, very young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~9.07 kpc) differs significantly from the median photometric distance (~4.42 kpc).

Distant High extinction Massive Very young

Data

🔍 Search references for FSR 0051 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	–	273.282	-13.365	0.11	-4.512	-6.595	–
Just et al.	2023	273.259	-13.326	–	–	–	–
Bica et al.	2019	273.272	-13.333	–	–	–	–
Kharchenko et al.	2016	273.259	-13.326	–	–	–	–
Kharchenko et al.	2013	273.267	-13.325	–	1.13	-9.43	–
Froebrich et al.	2007	273.267	-13.331	–	–	–	–
Dias et al.	2002	273.267	-13.331	–	0.48	0.09	–

💡 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	–	3622	–	–
Kharchenko et al.	2016	4.42	3.61	–	1	–	–	–	–
Kharchenko et al.	2013	4.42	3.61	–	1	–	–	–	–
Dias et al.	2002	4.42	3.61	–	1	–	–	–	–

Visualization

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