MWSC 5116

0.21 UTI

0.0

C_N

0.29

C_dens

0.25

C_C3

0.25

C_lit

1.0

C_dup

C3 classification BD

Number of members (P>50%) 23

Radius (P>50% members) 6.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.29 Loose
C_C3 0.25 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

ℹ️

MWSC 5116 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by low extinction. It is catalogued as an 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.

Relatively close Low extinction Old

Data

🔍 Search references for MWSC 5116 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	174.764	-36.354	0.479	-8.984	-0.21	35.479
Just et al.	2023	174.765	-36.337	–	–	–	–
Bica et al.	2019	174.766	-36.333	–	–	–	–
Kharchenko et al.	2016	174.765	-36.337	–	–	–	–
Schmeja et al.	2014	174.772	-36.34	–	-9.94	5.21	–

💡 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	–	–	–	3273	–	317	–	–
Kharchenko et al.	2016	1.62	0.48	–	3273	–	–	–	–
Schmeja et al.	2014	1.62	0.48	–	3273	–	–	–	–

Visualization

ℹ️