MWSC 5731

0.19 UTI

0.0

C_N

0.06

C_dens

0.38

C_C3

0.25

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 17

Radius (P>50% members) 7.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.38 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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MWSC 5731 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a massive, old cluster (see Parameters). It is poorly studied in the literature.

⚠️ 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.

Distant Moderate extinction Massive Old

Data

🔍 Search references for MWSC 5731 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	–	300.707	-16.207	0.295	-1.913	-3.687	-32.159
Just et al.	2023	300.701	-16.223	–	–	–	–
Bica et al.	2019	300.705	-16.226	–	–	–	–
Kharchenko et al.	2016	300.701	-16.223	–	–	–	–
Schmeja et al.	2014	300.708	-16.22	–	-1.96	-9.19	–

💡 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	–	–	–	1841	–	3266	–	–
Kharchenko et al.	2016	3.38	1.03	–	1841	–	–	–	–
Schmeja et al.	2014	3.38	1.03	–	1841	–	–	–	–

Visualization

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