CWWDL 11583

0.13 UTI

0.38

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.32

C_dup

C3 classification AB

Number of members (P>50%) 38

Radius (P>50% members) 2.8 [arcmin]

C_N 0.38 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.32 Possibly duplicate

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

Overview

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CWWDL 11583 is a poorly populated, very dense 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, 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 11583 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	–	298.145	32.537	0.406	-2.398	-5.385	-2.321
Chi et al.	2023	298.145	32.538	0.399	-2.31	-5.383	-2.321

💡 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	–	–	–	14	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 517	68.4	298.13	32.55	0.4	-2.4	-5.39	-2.32	0.03
UBC 1570	68.4	298.14	32.55	0.4	-2.4	-5.39	-2.32	0.5

💡 Note: The % column shows the percentage of members that CWWDL 11583 shares with each listed object.

Visualization

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