CWWDL 11597

0.06 UTI

0.49

C_N

0.89

C_dens

0.75

C_C3

0.0

C_lit

0.14

C_dup

N₅₀ (P>50% members) 49

Stellar density (N₅₀/rad) 4.5 [N/pc²]

C3 classification AB

C_N 0.49 Poorly populated
C_dens 0.89 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.14 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 11597 is a poorly populated, 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a significant percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 11597 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	99999–	298.302	32.652	0.474	-2.458	-3.457	-1.288
Chi et al.	2023	298.329	32.656	0.478	-2.431	-3.518	-1.288

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	18	0.320	–	–	–
Chi et al.	2023	–	–	–	18	0.320	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 46	85.7	298.31	32.65	0.47	-2.48	-3.44	10.05	0.56
CWWDL 14020	73.5	298.3	32.63	0.47	-2.46	-3.45	10.05	0.03
UBC 1079	67.3	298.32	32.66	0.48	-2.48	-3.45	10.05	0.02

💡 Note: The % column shows the percentage of members that CWWDL 11597 shares with each listed object.

Visualization

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