CWWDL 1993

0.08 UTI

0.0

C_N

0.13

C_dens

0.75

C_C3

0.0

C_lit

0.44

C_dup

C3 classification AB

Number of members (P>50%) 20

Radius (P>50% members) 6.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.13 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

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

Overview

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CWWDL 1993 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 1993 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	–	22.914	62.389	0.323	-1.558	-0.37	–
Chi et al.	2023	23.069	62.397	0.323	-1.55	-0.36	-71.413

💡 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	–	–	–	1	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0237	56.0	22.67	62.4	0.33	-1.59	-0.42	–	0.55

💡 Note: The % column shows the percentage of members that CWWDL 1993 shares with each listed object.

Visualization

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