MWSC 5029

0.07 UTI

0.0

C_N

0.11

C_dens

0.12

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 19

Core radius and density 1.5 [pc], 0.5 [pc^-2]

C3 classification CD

C_N 0.0 Sparse
C_dens 0.11 Very loose
C_C3 0.12 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 5029 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 an 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 Old

Data

🔍 Search references for MWSC 5029 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–	131.383	-11.63	0.388	-5.745	2.421	34.263
Just et al.	2023	131.401	-11.652	–	–	–	–
Bica et al.	2019	131.404	-11.652	–	–	–	–
Kharchenko et al.	2016	131.401	-11.652	–	–	–	–
Schmeja et al.	2014	131.407	-11.655	–	-2.86	3.0	–

💡 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–	1.95	0.46	–	1928	–	126	–	–
Just et al.	2023	–	–	–	1928	–	126	–	–
Kharchenko et al.	2016	1.95	0.46	–	1928	–	–	–	–
Schmeja et al.	2014	1.95	0.46	–	1928	–	–	–	–

Visualization

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