CWNU 4359

0.03 UTI

0.51

C_N

0.87

C_dens

1.0

C_C3

0.0

C_lit

0.06

C_dup

C3 classification AA

Number of members (P>50%) 52

Radius (P>50% members) 3.4 [arcmin]

C_N 0.51 Moderately populated
C_dens 0.87 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.06 Very likely duplicate

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

Overview

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CWNU 4359 is a moderately populated, dense object of very high 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 very 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 4359 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	–	222.384	-59.763	0.286	-4.628	-2.682	64.534
He et al.	2023	222.385	-59.752	0.273	-4.628	-2.676	122.07

💡 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	3.47	7.50	–	1	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2661	94.2	222.38	-59.77	0.3	-4.68	-2.7	18.53	0.53

💡 Note: The % column shows the percentage of members that CWNU 4359 shares with each listed object.

Visualization

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