CWWDL 439

0.14 UTI

0.38

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.37

C_dup

C3 classification BB

Number of members (P>50%) 38

Radius (P>50% members) 1.8 [arcmin]

C_N 0.38 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.37 Possibly duplicate

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

Overview

ℹ️

CWWDL 439 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a large distance, below the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

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

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 439 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	139.547	-53.272	0.19	-4.958	4.359	62.851
Chi et al.	2023	139.456	-53.239	0.211	-4.861	4.363	57.528

💡 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	–	–	–	71	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1461	63.2	139.56	-53.28	0.18	-5.06	4.35	71.24	0.58

💡 Note: The % column shows the percentage of members that CWWDL 439 shares with each listed object.

Visualization

ℹ️