CWNU 3766

0.01 UTI

0.29

C_N

0.69

C_dens

1.0

C_C3

0.0

C_lit

0.03

C_dup

C3 classification AA

Number of members (P>50%) 29

Radius (P>50% members) 2.0 [arcmin]

C_N 0.29 Poorly populated
C_dens 0.69 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

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CWNU 3766 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant Very high extinction Young

Data

🔍 Search references for CWNU 3766 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	–	293.173	19.303	0.201	-2.54	-5.427	30.296
He et al.	2023	293.168	19.3	0.204	-2.542	-5.432	17.36

💡 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	3.98	5.60	–	32	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 449	96.6	293.19	19.35	0.19	-2.5	-5.4	25.06	0.37

💡 Note: The % column shows the percentage of members that CWNU 3766 shares with each listed object.

Visualization

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