CWWDL 14366

0.02 UTI

0.51

C_N

0.34

C_dens

0.75

C_C3

0.0

C_lit

0.08

C_dup

C3 classification AB

Number of members (P>50%) 52

Radius (P>50% members) 17.3 [arcmin]

C_N 0.51 Moderately populated
C_dens 0.34 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

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

Overview

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CWWDL 14366 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a 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.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14366 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	–	348.219	57.477	0.916	0.242	-1.34	-29.865
Chi et al.	2023	348.309	57.522	0.908	0.241	-1.341	-24.291

💡 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	–	–	–	41	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 394	92.3	348.15	57.48	0.92	0.25	-1.35	-27.34	0.12
LISC 3420	50.0	348.1	57.47	0.91	0.26	-1.37	-31.89	0.24
Theia 2526	48.1	348.12	57.48	0.91	0.27	-1.37	-31.89	0.0
CWNU 415	44.2	347.86	57.41	0.91	0.24	-1.38	-23.5	0.04
CWNU 83	19.2	347.51	57.0	0.91	0.19	-1.4	-19.28	0.05

💡 Note: The % column shows the percentage of members that CWWDL 14366 shares with each listed object.

Visualization

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