CWNU 3833

0.04 UTI

0.38

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.1

C_dup

C3 classification AB

Number of members (P>50%) 38

Radius (P>50% members) 1.1 [arcmin]

C_N 0.38 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.1 Likely duplicate

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

Overview

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CWNU 3833 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High extinction Young

Data

🔍 Search references for CWNU 3833 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	–	225.486	-60.028	0.309	-3.856	-2.798	-31.913
He et al.	2023	225.49	-60.029	0.309	-3.861	-2.799	–

💡 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	2.63	3.85	–	25	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWL 1746	89.5	225.49	-60.03	0.31	-3.86	-2.8	-31.91	0.57

💡 Note: The % column shows the percentage of members that CWNU 3833 shares with each listed object.

Visualization

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