CWWDL 13359

0.03 UTI

0.0

C_N

0.12

C_dens

0.25

C_C3

0.0

C_lit

0.4

C_dup

C3 classification CC

Number of members (P>50%) 19

Radius (P>50% members) 9.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.12 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.4 Possibly duplicate

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

Overview

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CWWDL 13359 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate 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 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 Young

Data

🔍 Search references for CWWDL 13359 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	–	30.86	59.01	0.464	-0.809	-1.204	62.06
Chi et al.	2023	30.789	59.022	0.457	-0.83	-1.118	-38.756

💡 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	–	–	–	31	-0.180	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1235	60.0	30.88	59.0	0.46	-0.73	-1.31	-34.95	0.38
Theia 2252	48.0	30.94	58.99	0.46	-0.72	-1.32	-34.95	0.02

💡 Note: The % column shows the percentage of members that CWWDL 13359 shares with each listed object.

Visualization

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