CWWDL 14393

0.08 UTI

0.45

C_N

0.85

C_dens

0.75

C_C3

0.0

C_lit

0.2

C_dup

C3 classification AB

Number of members (P>50%) 45

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

C_N 0.45 Poorly populated
C_dens 0.85 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.2 Likely duplicate

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

Overview

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CWWDL 14393 is a poorly populated, dense 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, very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is 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 14393 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	–	262.719	-33.477	0.886	2.468	-1.911	0.065
Chi et al.	2023	262.68	-33.503	0.902	2.385	-1.893	-7.823

💡 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	–	–	–	1	0.370	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1645	80.0	262.75	-33.48	0.88	2.51	-1.92	-4.18	0.04
UFMG 77	80.0	262.79	-33.47	0.88	2.51	-1.9	0.07	0.46

💡 Note: The % column shows the percentage of members that CWWDL 14393 shares with each listed object.

Visualization

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