CWNU 3772

0.04 UTI

0.0

C_N

0.75

C_dens

0.38

C_C3

0.0

C_lit

0.16

C_dup

C3 classification CB

Number of members (P>50%) 23

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

C_N 0.0 Sparse
C_dens 0.75 Dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

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

Overview

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CWNU 3772 is a sparse, dense object of low C3 quality. Its parallax locates it at a moderate distance, near 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.

Distant Moderate extinction Very young

Data

🔍 Search references for CWNU 3772 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	–	7.501	62.843	0.235	-2.031	-0.423	-72.101
He et al.	2023	7.501	62.836	0.226	-2.037	-0.444	–

💡 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	3.89	2.90	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1851	84.0	7.51	62.84	0.23	-2.03	-0.42	-72.1	0.25

💡 Note: The % column shows the percentage of members that CWNU 3772 shares with each listed object.

Visualization

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