CWWDL 14593

0.11 UTI

0.0

C_N

0.51

C_dens

0.75

C_C3

0.0

C_lit

0.44

C_dup

N₅₀ (P>50% members) 24

Stellar density (N₅₀/rad) 2.6 [N/pc²]

C3 classification BA

C_N 0.0 Sparse
C_dens 0.51 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 14593 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a very 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry, and a moderate 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 14593 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–	123.099	-46.176	2.866	-6.514	9.405	15.286
Chi et al.	2023	123.185	-45.992	2.856	-6.502	9.444	16.414

💡 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	-0.280	–	–	–
Chi et al.	2023	–	–	–	1	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OCSN 254	56.0	122.38	-47.34	2.89	-6.4	9.6	14.61	0.07
Pozzo 1	48.0	122.39	-47.33	2.89	-6.41	9.61	15.22	1.0
CWWDL 14592	32.0	123.01	-46.3	2.79	-6.35	9.19	15.12	0.16

💡 Note: The % column shows the percentage of members that CWWDL 14593 shares with each listed object.

Visualization

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