CWNU 3682

0.11 UTI

0.5

C_N

0.29

C_dens

0.38

C_C3

0.0

C_lit

0.48

C_dup

C3 classification CB

Number of members (P>50%) 50

Radius (P>50% members) 3.2 [arcmin]

C_N 0.5 Moderately populated
C_dens 0.29 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.48 Possibly duplicate

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

Overview

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CWNU 3682 is a moderately populated, loose object of low C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as a 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.

Very distant High extinction Young

Data

🔍 Search references for CWNU 3682 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	–	315.491	46.442	0.159	-3.434	-3.86	-33.64
He et al.	2023	315.492	46.443	0.158	-3.429	-3.863	-53.55

💡 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
He et al.	2023	5.01	3.55	–	25	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2850	52.0	315.49	46.44	0.16	-3.44	-3.89	-33.64	0.15

💡 Note: The % column shows the percentage of members that CWNU 3682 shares with each listed object.

Visualization

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