CWNU 3826

0.17 UTI

0.45

C_N

0.88

C_dens

0.62

C_C3

0.0

C_lit

0.44

C_dup

C3 classification AC

Number of members (P>50%) 45

Radius (P>50% members) 3.5 [arcmin]

C_N 0.45 Poorly populated
C_dens 0.88 Dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

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

Overview

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CWNU 3826 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as an intermediate-age 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.

Relatively close High extinction Intermediate age

Data

🔍 Search references for CWNU 3826 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	–	20.847	66.972	0.318	-2.065	1.002	-72.652
He et al.	2023	20.863	66.974	0.322	-2.088	1.005	-67.09

💡 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	2.75	3.25	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1008	55.6	20.85	66.97	0.32	-2.07	1.01	-67.09	0.27

💡 Note: The % column shows the percentage of members that CWNU 3826 shares with each listed object.

Visualization

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