CWWDL 13945

0.00 UTI

0.4

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 40

Radius (P>50% members) 5.1 [arcmin]

C3 classification CB

C_N 0.4 Poorly populated
C_dens 1.0 Very 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 13945 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively 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 large 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 13945 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–	330.471	56.029	0.641	-2.004	-1.667	34.448
Chi et al.	2023	330.475	56.025	0.627	-2.014	-1.697	-14.965

💡 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–	–	–	–	10	-0.280	–	–	–
Chi et al.	2023	–	–	–	10	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 28	100.0	330.47	56.03	0.64	-2.01	-1.66	34.45	0.51
UBC 1154	100.0	330.47	56.04	0.64	-2.0	-1.67	34.45	0.01
CWWDL 14210	92.5	330.47	56.05	0.64	-1.98	-1.7	34.45	0.13

💡 Note: The % column shows the percentage of members that CWWDL 13945 shares with each listed object.

Visualization

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