CWWDL 14677

0.00 UTI

0.85

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 370

Radius (P>50% members) 94.8 [arcmin]

C_N 0.85 Rich
C_dens 1.0 Very dense
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

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CWWDL 14677 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, 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.

Very close Low extinction Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14677 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	–	1.027	-30.006	4.228	18.751	2.613	5.525
Wei et al.	2025	1.356	-29.982	4.219	18.742	2.372	–
Chi et al.	2023	0.953	-30.002	4.223	18.721	2.611	3.682

💡 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
Wei et al.	2025	0.30	0.62	–	52	-0.250	623	0.28	–
Chi et al.	2023	–	–	–	5	0.070	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Blanco 1	100.0	1.22	-29.95	4.23	18.75	2.6	5.19	1.0
Dzeta Scul	4.1	0.43	-30.2	4.21	18.72	2.39	6.9	0.12

💡 Note: The % column shows the percentage of members that CWWDL 14677 shares with each listed object.

Visualization

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