CWWDL 14038

0.04 UTI

0.27

C_N

0.21

C_dens

0.25

C_C3

0.0

C_lit

0.3

C_dup

N₅₀ (P>50% members) 27

Stellar density (N₅₀/rad) 1.0 [N/pc²]

C3 classification DB

C_N 0.27 Poorly populated
C_dens 0.21 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.3 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 14038 is a poorly populated, very loose object of low 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry, and a very small 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 14038 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	99999–	94.737	23.158	0.521	0.48	-1.582	-1.826
Chi et al.	2023	94.83	23.165	0.513	0.512	-1.623	–

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	1	0.230	–	–	–
Chi et al.	2023	–	–	–	1	0.230	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1306	70.4	94.62	22.88	0.53	0.45	-1.62	-1.83	0.21
Collinder 89	59.3	94.72	23.2	0.52	0.45	-1.54	-1.83	0.57
CWWDL 14032	7.4	94.5	22.65	0.53	0.42	-1.66	-32.33	0.05

💡 Note: The % column shows the percentage of members that CWWDL 14038 shares with each listed object.

Visualization

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