CWNU 3933

0.06 UTI

0.54

C_N

0.15

C_dens

0.75

C_C3

0.0

C_lit

0.21

C_dup

N_m (P>50%) 58

Core radius and density 3.3 [pc], 0.8 [pc^-2]

C3 classification AB

C_N 0.54 Moderately populated
C_dens 0.15 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.21 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3933 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a very large distance, above the mid-plane, affected by very high extinction. It is catalogued as a very 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.

Very distant Very high extinction Very young

Data

🔍 Search references for CWNU 3933 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	99999–	289.866	14.901	0.099	-3.149	-6.391	34.563
He et al.	2023	289.866	14.901	0.102	-3.157	-6.384	34.37

💡 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]	B_frac	BSS
UCC	99999–	7.41	7.3	–	16	–	–	–	–
He et al.	2023	7.41	7.30	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Juchert J1919.4+1453	79.3	289.87	14.91	0.1	-3.16	-6.38	34.76	0.33

💡 Note: The % column shows the percentage of members that CWNU 3933 shares with each listed object.

Visualization

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