CWNU 4445

0.20 UTI

0.0

C_N

0.37

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 24

Core radius and density 0.6 [pc], 1.8 [pc^-2]

C3 classification AC

C_N 0.0 Sparse
C_dens 0.37 Loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 4445 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a close 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: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Very high extinction Very young

Data

🔍 Search references for CWNU 4445 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	99999–	345.295	61.747	1.234	-0.938	-2.367	-24.791
He et al.	2023	345.315	61.747	1.236	-0.897	-2.392	-31.25

💡 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]	B_frac	BSS
UCC	99999–	0.85	5.3	–	8	–	–	–	–
He et al.	2023	0.85	5.30	–	8	–	–	–	–

Visualization

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