MWSC 5295

0.14 UTI

0.0

C_N

0.18

C_dens

0.0

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 22

Stellar density (N₅₀/rad) 0.9 [N/pc²]

C3 classification DD

C_N 0.0 Sparse
C_dens 0.18 Very loose
C_C3 0.0 Very low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

MWSC 5295 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 poorly studied in the literature.

(*): The parallax distance estimate (~2.56 kpc) differs significantly from the median photometric distance (~1.76 kpc).

⚠️ 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 5295 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	233.691	-13.389	0.39	-8.311	-1.384	-120.658
Just et al.	2023	233.655	-13.379	–	–	–	–
Bica et al.	2019	233.651	-13.375	–	–	–	–
Kharchenko et al.	2016	233.655	-13.379	–	–	–	–
Schmeja et al.	2014	233.662	-13.38	–	-4.26	-4.5	–

💡 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–	1.76	0.64	–	2291	–	485	–	–
Just et al.	2023	–	–	–	2291	–	485	–	–
Kharchenko et al.	2016	1.76	0.64	–	2291	–	–	–	–
Schmeja et al.	2014	1.76	0.64	–	2291	–	–	–	–

Visualization

ℹ️