CWWDL 14433

0.00 UTI

0.75

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%) 108

Radius (P>50% members) 12.8 [arcmin]

C_N 0.75 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 14433 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a near-solar metallicity, very 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, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14433 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	–	256.514	-35.073	0.91	1.257	-2.17	1.462
Chi et al.	2023	256.593	-35.049	0.915	1.224	-2.138	1.821

💡 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	–	–	–	2	0.070	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Gulliver 29	100.0	256.67	-35.26	0.9	1.28	-2.2	5.0	0.74
CWWDL 14471	35.2	256.42	-35.15	0.93	1.2	-2.17	0.25	0.01

💡 Note: The % column shows the percentage of members that CWWDL 14433 shares with each listed object.

Visualization

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