MWSC 5088

0.03 UTI

0.0

C_N

0.02

C_dens

0.0

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 24

Core radius and density 5.5 [pc], 0.1 [pc^-2]

C3 classification DD

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.0 Very low quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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MWSC 5088 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by low extinction. It is catalogued as a massive, old cluster (see Parameters). It is rarely 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 Massive Old

Data

🔍 Search references for MWSC 5088 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–	167.263	-32.526	0.339	-6.005	-2.043	37.974
Just et al.	2023	167.178	-32.526	–	–	–	–
Bica et al.	2019	167.176	-32.522	–	–	–	–
Kharchenko et al.	2016	167.178	-32.526	–	–	–	–
Schmeja et al.	2014	167.185	-32.53	–	-7.82	0.86	–

💡 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–	2.83	0.39	–	1679	–	1186	–	–
Just et al.	2023	–	–	–	1679	–	1186	–	–
Kharchenko et al.	2016	2.83	0.39	–	1679	–	–	–	–
Schmeja et al.	2014	2.83	0.39	–	1679	–	–	–	–

Visualization

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