CWWDL 2006

0.08 UTI

0.0

C_N

0.02

C_dens

0.62

C_C3

0.0

C_lit

0.6

C_dup

C3 classification AC

Number of members (P>50%) 17

Radius (P>50% members) 13.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.6 Likely unique

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

Overview

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CWWDL 2006 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 2006 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	–	28.916	61.987	0.329	-1.067	-0.306	–
Chi et al.	2023	29.012	62.039	0.314	-1.075	-0.3	-60.569

💡 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	-0.040	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 414	40.0	28.48	61.98	0.32	-1.03	-0.28	–	0.23
Berkeley 7	12.0	28.55	62.37	0.34	-0.98	-0.21	-67.13	0.9
HSC 1060	12.0	29.52	61.91	0.34	-1.03	-0.39	-15.47	0.14
CWWDL 8417	8.0	28.64	61.78	0.35	-1.12	-0.39	–	0.11

💡 Note: The % column shows the percentage of members that CWWDL 2006 shares with each listed object.

Visualization

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