CWNU 3718

0.05 UTI

0.35

C_N

0.37

C_dens

0.5

C_C3

0.0

C_lit

0.2

C_dup

C3 classification BB

Number of members (P>50%) 35

Radius (P>50% members) 5.6 [arcmin]

C_N 0.35 Poorly populated
C_dens 0.37 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.2 Likely duplicate

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

Overview

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CWNU 3718 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate 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.

Relatively close Moderate extinction Very young

Data

🔍 Search references for CWNU 3718 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	–	108.292	-8.372	0.375	-1.051	1.018	-14.542
He et al.	2023	108.297	-8.362	0.379	-1.06	1.012	-14.54

💡 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	2.51	1.05	–	6	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1753	80.0	108.29	-8.39	0.38	-1.05	1.02	-14.54	0.17

💡 Note: The % column shows the percentage of members that CWNU 3718 shares with each listed object.

Visualization

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