CWWDL 14632

0.00 UTI

0.3

C_N

0.76

C_dens

0.38

C_C3

0.0

C_lit

0.0

C_dup

C3 classification CB

Number of members (P>50%) 30

Radius (P>50% members) 16.3 [arcmin]

C_N 0.3 Poorly populated
C_dens 0.76 Dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWWDL 14632 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a 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, and a significant percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14632 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	–	288.603	14.349	1.687	2.423	1.056	-6.697
Chi et al.	2023	288.759	14.398	1.74	2.436	1.081	-5.931

💡 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	–	–	–	66	0.160	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 53	100.0	288.52	14.37	1.68	2.45	1.02	-5.7	0.79
CWWDL 14443	56.7	288.5	14.27	1.66	2.44	0.99	-5.64	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14632 shares with each listed object.

Visualization

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