CWWDL 3307

0.00 UTI

0.39

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 39

Stellar density (N₅₀/rad) 8.3 [N/pc²]

C3 classification AB

C_N 0.39 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 3307 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below 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 very likely a duplicate object, which shares a large 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 3307 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–	27.486	53.894	0.336	-0.792	-1.64	-97.287
Chi et al.	2023	27.471	53.882	0.33	-0.818	-1.591	-97.287

💡 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–	–	–	–	1	0.440	–	–	–
Chi et al.	2023	–	–	–	1	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 188	100.0	27.49	53.9	0.33	-0.83	-1.59	-70.26	0.27
SAI 15	97.4	27.49	53.9	0.34	-0.82	-1.62	-97.29	0.46

💡 Note: The % column shows the percentage of members that CWWDL 3307 shares with each listed object.

Visualization

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