MWSC 5215

0.38 UTI

0.55

C_N

0.25

C_dens

0.62

C_C3

0.25

C_lit

1.0

C_dup

C3 classification AC

Number of members (P>50%) 59

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

C_N 0.55 Moderately populated
C_dens 0.25 Loose
C_C3 0.62 Intermediate 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 5215 is a moderately populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate^* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as a massive, old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.26 kpc) differs significantly from the median photometric distance (~3.12 kpc).

Distant Moderate extinction Massive Old

Data

🔍 Search references for MWSC 5215 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	206.482	-41.855	0.235	-5.226	-1.356	–
Just et al.	2023	206.504	-41.84	–	–	–	–
Bica et al.	2019	206.499	-41.838	–	–	–	–
Kharchenko et al.	2016	206.504	-41.84	–	–	–	–
Schmeja et al.	2014	206.512	-41.843	–	-5.67	-0.57	–

💡 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	–	–	–	1950	–	1374	–	–
Kharchenko et al.	2016	3.12	1.26	–	1950	–	–	–	–
Schmeja et al.	2014	3.12	1.26	–	1950	–	–	–	–

Visualization

ℹ️