CWWDL 214

0.00 UTI

0.41

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 41

Radius (P>50% members) 2.0 [arcmin]

C_N 0.41 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

ℹ️

CWWDL 214 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWDL 214 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	149.032	-60.18	0.33	-5.892	5.212	1.812
Chi et al.	2023	149.032	-60.164	0.328	-5.951	5.182	0.093

💡 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
Chi et al.	2023	–	–	–	302	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 676	100.0	149.03	-60.18	0.33	-5.88	5.22	-0.08	0.54
OC 0534	100.0	149.03	-60.18	0.33	-5.88	5.22	0.81	0.02
Theia 6242	100.0	149.03	-60.18	0.33	-5.87	5.22	0.66	0.04

💡 Note: The % column shows the percentage of members that CWWDL 214 shares with each listed object.

Visualization

ℹ️