CWNU 3785

0.07 UTI

0.52

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.18

C_dup

C3 classification CB

Number of members (P>50%) 54

Radius (P>50% members) 2.7 [arcmin]

C_N 0.52 Moderately populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.18 Likely duplicate

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

Overview

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CWNU 3785 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near 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 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 Intermediate age

Data

🔍 Search references for CWNU 3785 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	–	279.69	-6.568	0.424	0.337	-1.512	4.897
He et al.	2023	279.69	-6.573	0.432	0.327	-1.518	89.93

💡 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	1.91	4.40	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 249	81.5	279.69	-6.57	0.42	0.34	-1.51	89.93	0.34

💡 Note: The % column shows the percentage of members that CWNU 3785 shares with each listed object.

Visualization

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