CWWDL 11734

0.12 UTI

0.63

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.24

C_dup

C3 classification AA

Number of members (P>50%) 76

Radius (P>50% members) 3.5 [arcmin]

C_N 0.63 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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CWWDL 11734 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above 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 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 11734 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	–	11.329	64.367	0.321	-2.427	-0.373	–
Chi et al.	2023	11.756	64.328	0.35	-2.38	-0.403	-61.763

💡 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	–	–	–	58	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Berkeley 4	76.3	11.3	64.39	0.31	-2.4	-0.31	-60.44	0.91
OC 0230	31.6	11.28	64.38	0.32	-2.44	-0.36	–	0.0
OC 0229	19.7	11.28	64.39	0.3	-2.43	-0.34	–	0.0

💡 Note: The % column shows the percentage of members that CWWDL 11734 shares with each listed object.

Visualization

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