CWWDL 13510

0.05 UTI

0.49

C_N

0.94

C_dens

0.75

C_C3

0.0

C_lit

0.12

C_dup

C3 classification AB

Number of members (P>50%) 49

Radius (P>50% members) 5.3 [arcmin]

C_N 0.49 Poorly populated
C_dens 0.94 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

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

Overview

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CWWDL 13510 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a large percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 13510 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	–	19.857	61.007	0.477	-1.248	-0.222	–
Chi et al.	2023	19.89	60.98	0.467	-1.233	-0.219	-11.826

💡 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	–	–	–	38	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 39	87.8	19.85	61.02	0.48	-1.25	-0.21	–	0.61
CWWDL 6218	75.5	19.82	61.03	0.5	-1.25	-0.21	–	0.03
OC 0235	61.2	19.82	61.02	0.49	-1.23	-0.22	–	0.0

💡 Note: The % column shows the percentage of members that CWWDL 13510 shares with each listed object.

Visualization

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