CWWDL 13583

0.16 UTI

0.42

C_N

0.56

C_dens

0.75

C_C3

0.0

C_lit

0.48

C_dup

C3 classification AB

Number of members (P>50%) 42

Radius (P>50% members) 5.7 [arcmin]

C_N 0.42 Poorly populated
C_dens 0.56 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.48 Possibly duplicate

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

Overview

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CWWDL 13583 is a poorly populated, moderately dense 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, 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, 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 13583 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	–	177.882	-62.655	0.428	-5.591	0.754	-13.233
Chi et al.	2023	177.928	-62.645	0.445	-5.583	0.819	4.121

💡 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	–	–	–	54	0.070	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 280	52.4	177.95	-62.66	0.42	-5.61	0.72	-11.96	0.57
CWWDL 13421	2.4	177.94	-62.99	0.43	-5.65	0.8	–	0.09

💡 Note: The % column shows the percentage of members that CWWDL 13583 shares with each listed object.

Visualization

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