CWWDL 6005

0.00 UTI

0.5

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.0

C_dup

C3 classification CA

Number of members (P>50%) 51

Radius (P>50% members) 3.9 [arcmin]

C_N 0.5 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate 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 6005 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively 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. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 6005 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	–	323.995	50.492	0.535	-3.827	-3.336	-2.883
Chi et al.	2023	324.0	50.504	0.53	-3.746	-3.31	27.543

💡 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	–	–	–	25	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 227	100.0	324.0	50.49	0.54	-3.84	-3.34	-33.31	0.05
UBC 1141	96.1	324.0	50.49	0.54	-3.84	-3.34	-33.31	0.43
Theia 3986	94.1	324.0	50.49	0.54	-3.84	-3.34	-2.88	0.0

💡 Note: The % column shows the percentage of members that CWWDL 6005 shares with each listed object.

Visualization

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