CWWDL 14289

0.00 UTI

0.5

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BA

Number of members (P>50%) 50

Radius (P>50% members) 9.4 [arcmin]

C_N 0.5 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 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 14289 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, 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. See table with shared members information.

(*): The parallax distance estimate (~0.57 kpc) differs significantly from the median photometric distance (~2.14 kpc).

Relatively close Moderate extinction Metal-poor Very young

Data

🔍 Search references for CWWDL 14289 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	–	91.685	-2.005	1.743	-0.661	-0.239	40.105
Wei et al.	2025	91.739	-2.033	1.733	-0.645	-0.292	–
Chi et al.	2023	91.719	-2.02	1.768	-0.546	-0.301	40.266

💡 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	2.14	2.65	–	13	-2.000	229	0.31	–
Chi et al.	2023	–	–	–	2	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 2184	100.0	91.72	-2.04	1.73	-0.66	-0.24	40.14	0.95
Theia 1408	100.0	91.7	-2.04	1.74	-0.66	-0.24	40.07	0.05

💡 Note: The % column shows the percentage of members that CWWDL 14289 shares with each listed object.

Visualization

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