CWWDL 14294

0.06 UTI

0.8

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.11

C_dup

C3 classification AA

Number of members (P>50%) 223

Radius (P>50% members) 19.1 [arcmin]

C_N 0.8 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.11 Likely duplicate

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

Overview

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CWWDL 14294 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, very young 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.

Close Low extinction Massive Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14294 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	–	105.752	-26.5	1.256	-3.225	3.51	32.701
Wei et al.	2025	105.828	-26.399	1.255	-3.284	3.491	–
Chi et al.	2023	105.768	-26.505	1.26	-3.257	3.516	32.374

💡 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	0.73	0.35	–	34	-0.250	1144	0.55	–
Chi et al.	2023	–	–	–	2	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Alessi 33	89.2	105.74	-26.48	1.25	-3.23	3.5	33.1	0.96
OC 0408	5.8	105.12	-26.51	1.22	-3.22	3.55	34.95	0.09
OC 0410	3.6	105.73	-27.38	1.2	-3.1	3.48	35.18	0.13

💡 Note: The % column shows the percentage of members that CWWDL 14294 shares with each listed object.

Visualization

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