CWWDL 12017

0.13 UTI

0.45

C_N

0.27

C_dens

0.75

C_C3

0.0

C_lit

0.44

C_dup

C3 classification AB

Number of members (P>50%) 45

Radius (P>50% members) 4.9 [arcmin]

C_N 0.45 Poorly populated
C_dens 0.27 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 12017 is a poorly populated, loose object of 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 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 12017 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	–	110.467	-6.539	0.248	-1.105	0.812	70.177
Chi et al.	2023	110.475	-6.556	0.249	-1.117	0.705	68.617

💡 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	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1356	55.6	110.46	-6.54	0.25	-1.09	0.83	70.18	0.25

💡 Note: The % column shows the percentage of members that CWWDL 12017 shares with each listed object.

Visualization

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