CWWDL 12514

0.00 UTI

0.6

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.0

C_dup

C3 classification CB

Number of members (P>50%) 69

Radius (P>50% members) 4.0 [arcmin]

C_N 0.6 Moderately populated
C_dens 1.0 Very dense
C_C3 0.38 Low 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

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CWWDL 12514 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a metal-poor, young 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.

Metal-poor Young

Data

🔍 Search references for CWWDL 12514 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	–	83.639	37.233	0.412	0.918	-2.49	–
Chi et al.	2023	83.633	37.217	0.418	0.891	-2.469	-3.299

💡 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	–	–	–	23	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1280	100.0	83.65	37.22	0.41	0.92	-2.49	26.19	0.55
CWNU 465	88.4	83.64	37.24	0.41	0.91	-2.5	–	0.0
CWNU 470	71.0	83.59	37.22	0.44	0.94	-2.48	26.41	0.13

💡 Note: The % column shows the percentage of members that CWWDL 12514 shares with each listed object.

Visualization

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