CWWDL 13504

0.04 UTI

0.0

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.16

C_dup

C3 classification CB

Number of members (P>50%) 24

Radius (P>50% members) 3.4 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

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

Overview

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CWWDL 13504 is a sparse, very dense object of low 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 likely a duplicate object, which shares a large 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 13504 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	356.852	60.505	0.469	-2.66	-2.023	-27.35
Chi et al.	2023	356.883	60.51	0.469	-2.596	-1.972	-21.664

💡 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	–	–	–	200	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Majaess 227	84.0	356.85	60.5	0.47	-2.66	-2.02	-27.35	0.46
UBC 1188	84.0	356.86	60.5	0.47	-2.66	-2.02	-27.35	0.04

💡 Note: The % column shows the percentage of members that CWWDL 13504 shares with each listed object.

Visualization

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