MWSC 4330

0.13 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.25

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 17

Radius (P>50% members) 5.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.12 Very 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 4330 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~7.04 kpc) differs significantly from the median photometric distance (~1.43 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 Moderate extinction Intermediate age

Data

🔍 Search references for MWSC 4330 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	259.292	-15.041	0.142	-3.859	-3.966	-79.207
Just et al.	2023	259.251	-15.08	–	–	–	–
Bica et al.	2019	259.258	-15.075	–	–	–	–
Kharchenko et al.	2016	259.251	-15.08	–	–	–	–
Scholz et al.	2015	259.26	-15.08	–	-2.92	-4.4	–

💡 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	–	–	–	355	–	98	–	–
Kharchenko et al.	2016	1.43	2.58	–	355	–	–	–	–
Scholz et al.	2015	1.43	2.58	–	355	–	–	–	–

Visualization

ℹ️