CWWDL 2073

0.04 UTI

0.0

C_N

0.31

C_dens

0.38

C_C3

0.0

C_lit

0.28

C_dup

C3 classification CB

Number of members (P>50%) 19

Radius (P>50% members) 4.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.31 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

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

Overview

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CWWDL 2073 is a sparse, loose object of low 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.

⚠️ 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 Young

Data

🔍 Search references for CWWDL 2073 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	–	113.505	-19.167	0.358	-1.81	2.61	42.59
Chi et al.	2023	113.505	-19.198	0.349	-1.857	2.516	40.575

💡 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	–	–	–	66	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 79	72.0	113.51	-19.19	0.36	-1.77	2.68	42.27	0.07
UBC 1378	68.0	113.51	-19.18	0.36	-1.78	2.69	42.43	0.56
UBC 1379	52.0	113.51	-19.19	0.35	-1.77	2.7	42.27	0.44

💡 Note: The % column shows the percentage of members that CWWDL 2073 shares with each listed object.

Visualization

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