CWWDL 14458

0.05 UTI

0.26

C_N

0.3

C_dens

0.38

C_C3

0.0

C_lit

0.27

C_dup

C3 classification CB

Number of members (P>50%) 26

Radius (P>50% members) 12.8 [arcmin]

C_N 0.26 Poorly populated
C_dens 0.3 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.27 Possibly duplicate

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

Overview

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CWWDL 14458 is a poorly populated, 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. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14458 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	–	52.538	59.803	0.894	-2.007	-0.754	-10.744
Chi et al.	2023	52.67	59.819	0.887	-2.057	-0.759	–

💡 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	–	–	–	4	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1722	96.2	52.68	59.96	0.9	-1.96	-0.7	-18.92	0.29
CWNU 1070	73.1	52.68	59.82	0.9	-1.96	-0.75	-27.48	0.29
CWNU 1058	53.8	51.4	60.1	0.89	-2.06	-0.73	-9.57	0.35

💡 Note: The % column shows the percentage of members that CWWDL 14458 shares with each listed object.

Visualization

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