CWWDL 14647

0.00 UTI

0.29

C_N

0.5

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AB

Number of members (P>50%) 29

Radius (P>50% members) 24.5 [arcmin]

C_N 0.29 Poorly populated
C_dens 0.5 Moderately dense
C_C3 0.75 High 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 14647 is a poorly populated, 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 very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a small 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 14647 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	–	279.984	0.642	2.089	2.516	-8.254	-7.701
Chi et al.	2023	280.017	0.696	2.075	2.558	-8.266	-8.749

💡 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	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 41	100.0	279.58	0.42	2.09	2.63	-8.29	-5.04	0.69
OC 0062	27.6	279.39	0.44	2.06	2.55	-8.24	1.1	0.0
CWWDL 14646	20.7	279.45	-0.34	2.13	2.75	-8.43	0.18	0.0
OC 0059	6.9	279.46	-0.37	2.14	2.83	-8.45	2.52	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14647 shares with each listed object.

Visualization

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