MWSC 5058

0.30 UTI

1.0

C_N

0.01

C_dens

0.5

C_C3

0.0

C_lit

1.0

C_dup

C3 classification DA

Number of members (P>50%) 564

Radius (P>50% members) 3.5 [arcmin]

C_N 1.0 Very rich
C_dens 0.01 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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MWSC 5058 is a very rich, very loose object of intermediate C3 quality. Its parallax locates it at a very large^* distance, well above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~-29.85 kpc) differs significantly from the median photometric distance (~1.19 kpc).

Relatively close Low extinction Intermediate age

Data

🔍 Search references for MWSC 5058 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	–	152.115	12.307	-0.034	-0.034	-0.127	–
Just et al.	2023	152.066	12.322	–	–	–	–
Schmeja et al.	2014	152.073	12.318	–	2.38	-3.81	–

💡 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	–	–	–	891	–	105	–	–
Schmeja et al.	2014	1.19	0.19	–	891	–	–	–	–

Visualization

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