CWWDL 14402

0.00 UTI

0.62

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%) 74

Radius (P>50% members) 9.9 [arcmin]

C_N 0.62 Moderately populated
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 14402 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, 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.

(*): The parallax distance estimate (~1.17 kpc) differs significantly from the median photometric distance (~1.87 kpc).

Relatively close Moderate extinction Massive Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14402 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	–	299.052	26.476	0.854	-1.002	-4.355	-11.676
Wei et al.	2025	299.135	26.547	0.854	-1.0	-4.365	–
Chi et al.	2023	299.11	26.505	0.868	-0.993	-4.345	-19.482

💡 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	1.87	2.12	–	135	-0.250	1308	0.52	–
Chi et al.	2023	–	–	–	4	0.320	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 129	100.0	299.07	26.45	0.85	-0.99	-4.36	-9.13	0.78

💡 Note: The % column shows the percentage of members that CWWDL 14402 shares with each listed object.

Visualization

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