CWWDL 14662

0.00 UTI

0.31

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 31

Stellar density (N₅₀/rad) 7.9 [N/pc²]

C3 classification BA

C_N 0.31 Poorly 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

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

Overview

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CWWDL 14662 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a very 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 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 Very young

Data

🔍 Search references for CWWDL 14662 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–	293.698	32.1	2.408	2.678	-1.327	-20.771
Chi et al.	2023	293.661	32.148	2.42	2.645	-1.344	-20.43

💡 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–	–	–	–	4	-0.100	–	–	–
Chi et al.	2023	–	–	–	4	-0.100	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 347	100.0	293.63	32.16	2.38	2.53	-1.31	-20.97	0.45
Theia 253	100.0	293.63	32.11	2.35	2.44	-1.33	-19.42	0.14

💡 Note: The % column shows the percentage of members that CWWDL 14662 shares with each listed object.

Visualization

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