CWNU 3751

0.03 UTI

0.34

C_N

0.26

C_dens

0.5

C_C3

0.0

C_lit

0.15

C_dup

C3 classification BB

Number of members (P>50%) 34

Radius (P>50% members) 6.3 [arcmin]

C_N 0.34 Poorly populated
C_dens 0.26 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.15 Likely duplicate

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

Overview

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CWNU 3751 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near 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.

Distant Very high extinction Very young

Data

🔍 Search references for CWNU 3751 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	–	277.799	-10.895	0.357	0.029	-1.965	38.491
He et al.	2023	277.795	-10.88	0.353	0.016	-1.962	–

💡 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	3.39	6.30	–	5	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 221	85.3	277.79	-10.88	0.36	0.0	-1.97	38.49	0.43

💡 Note: The % column shows the percentage of members that CWNU 3751 shares with each listed object.

Visualization

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