CWWDL 14285

0.00 UTI

0.33

C_N

0.46

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 33

Radius (P>50% members) 21.6 [arcmin]

C_N 0.33 Poorly populated
C_dens 0.46 Loose
C_C3 1.0 Very 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 14285 is a poorly populated, loose object of very high C3 quality. Its parallax locates it at a close distance, below 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. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14285 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	–	343.7	43.125	1.66	-0.539	-4.025	-9.301
Chi et al.	2023	343.706	43.187	1.669	-0.598	-4.02	-11.365

💡 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	–	–	–	3	-0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 165	100.0	343.79	43.29	1.66	-0.52	-4.0	-10.62	0.0
UPK 168	100.0	343.75	43.32	1.67	-0.53	-4.0	-9.91	0.85

💡 Note: The % column shows the percentage of members that CWWDL 14285 shares with each listed object.

Visualization

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