CWWDL 12541

0.00 UTI

0.0

C_N

0.25

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 24

Radius (P>50% members) 4.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.25 Loose
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 12541 is a sparse, loose object of very high C3 quality. Its parallax locates it at a moderate distance, above 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 very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a large percentage with at least one entry reported in the same catalogue. See table with shared members information.

Metal-poor Intermediate age

Data

🔍 Search references for CWWDL 12541 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	107.354	0.531	0.281	-1.003	-0.662	–
Chi et al.	2023	107.342	0.533	0.265	-0.888	-0.582	70.137

💡 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	–	–	–	100	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1344	100.0	107.35	0.54	0.28	-1.01	-0.68	59.45	0.5
CWWDL 12546	80.0	107.35	0.53	0.3	-1.0	-0.67	59.45	0.0
CWNU 192	72.0	107.35	0.53	0.3	-1.02	-0.68	–	0.0

💡 Note: The % column shows the percentage of members that CWWDL 12541 shares with each listed object.

Visualization

ℹ️