CWWDL 10501

0.09 UTI

0.4

C_N

0.14

C_dens

0.5

C_C3

0.0

C_lit

0.45

C_dup

C3 classification BB

Number of members (P>50%) 40

Radius (P>50% members) 12.2 [arcmin]

C_N 0.4 Poorly populated
C_dens 0.14 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.45 Possibly duplicate

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

Overview

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CWWDL 10501 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above 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 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 Very young

Data

🔍 Search references for CWWDL 10501 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	–	4.332	63.557	0.47	-3.163	-1.096	-81.844
Chi et al.	2023	4.206	63.55	0.471	-3.147	-1.105	-81.844

💡 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	–	–	–	2	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1201	55.0	3.83	63.56	0.47	-3.22	-1.11	-65.49	0.26
UBC 1203	40.0	4.71	63.58	0.47	-3.11	-1.05	-81.84	0.29
Theia 2330	32.5	3.77	63.56	0.47	-3.21	-1.1	-65.49	0.02
Casado 17	27.5	3.83	63.57	0.47	-3.23	-1.08	-65.49	0.24

💡 Note: The % column shows the percentage of members that CWWDL 10501 shares with each listed object.

Visualization

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