CWWDL 2025

0.09 UTI

0.51

C_N

0.49

C_dens

0.5

C_C3

0.0

C_lit

0.29

C_dup

C3 classification BB

Number of members (P>50%) 52

Radius (P>50% members) 3.5 [arcmin]

C_N 0.51 Moderately populated
C_dens 0.49 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.29 Possibly duplicate

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

Overview

ℹ️

CWWDL 2025 is a moderately populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a metal-poor, intermediate-age 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.

Metal-poor Intermediate age

Data

🔍 Search references for CWWDL 2025 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	75.186	41.241	0.221	0.332	-1.285	-59.113
Chi et al.	2023	75.093	41.35	0.256	0.373	-1.404	-18.773

💡 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	–	–	–	151	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
SAI 40	71.2	75.21	41.22	0.21	0.29	-1.22	-16.52	0.63
UBC 431	59.6	75.22	41.22	0.2	0.31	-1.2	-16.52	0.02

💡 Note: The % column shows the percentage of members that CWWDL 2025 shares with each listed object.

Visualization

ℹ️