CWWDL 13288

0.07 UTI

0.0

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.24

C_dup

N₅₀ (P>50% members) 21

Stellar density (N₅₀/rad) 5.7 [N/pc²]

C3 classification CB

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 13288 is a sparse, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, below 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 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 Young

Data

🔍 Search references for CWWDL 13288 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–	3.39	53.823	0.513	-2.188	-1.101	–
Chi et al.	2023	3.401	53.844	0.5	-2.212	-1.134	-47.909

💡 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–	–	–	–	81	0.350	–	–	–
Chi et al.	2023	–	–	–	81	0.350	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 596	76.0	3.38	53.83	0.51	-2.2	-1.04	–	0.36

💡 Note: The % column shows the percentage of members that CWWDL 13288 shares with each listed object.

Visualization

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