CWWDL 11968

0.06 UTI

0.45

C_N

1.0

C_dens

0.12

C_C3

0.0

C_lit

0.2

C_dup

C3 classification DC

Number of members (P>50%) 45

Radius (P>50% members) 2.4 [arcmin]

C_N 0.45 Poorly populated
C_dens 1.0 Very dense
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.2 Likely duplicate

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

Overview

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CWWDL 11968 is a poorly populated, very dense object of very low 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 11968 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	–	100.613	12.868	0.342	0.816	-1.512	–
Chi et al.	2023	100.603	12.877	0.329	0.819	-1.541	86.476

💡 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	–	–	–	44	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1321	80.0	100.62	12.87	0.35	0.81	-1.51	–	0.48

💡 Note: The % column shows the percentage of members that CWWDL 11968 shares with each listed object.

Visualization

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