CWWDL 13357

0.01 UTI

0.42

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.02

C_dup

N₅₀ (P>50% members) 42

Stellar density (N₅₀/rad) 5.7 [N/pc²]

C3 classification AB

C_N 0.42 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.02 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 13357 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close 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 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 Young

Data

🔍 Search references for CWWDL 13357 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–	335.556	54.555	0.663	1.693	-2.306	-9.347
Chi et al.	2023	335.585	54.564	0.658	1.746	-2.368	-8.675

💡 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–	–	–	–	54	0.350	–	–	–
Chi et al.	2023	–	–	–	54	0.350	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 4535	100.0	335.54	54.55	0.66	1.68	-2.29	-12.31	0.09
HXHWL 23	97.6	335.54	54.56	0.66	1.68	-2.29	-12.31	0.46

💡 Note: The % column shows the percentage of members that CWWDL 13357 shares with each listed object.

Visualization

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