CWNU 4205

0.19 UTI

0.55

C_N

0.39

C_dens

0.75

C_C3

0.0

C_lit

0.58

C_dup

N₅₀ (P>50% members) 59

Stellar density (N₅₀/rad) 1.9 [N/pc²]

C3 classification AB

C_N 0.55 Moderately populated
C_dens 0.39 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.58 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 4205 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a very large distance, above the mid-plane, affected by very high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Extremely distant Very high extinction Intermediate age

Data

🔍 Search references for CWNU 4205 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–	302.773	36.148	0.09	-2.355	-3.883	-58.197
He et al.	2023	302.768	36.151	0.076	-2.355	-3.871	-60.64

💡 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–	11.48	5.2	–	126	–	–	–	–
He et al.	2023	11.48	5.20	–	126	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 583	42.4	302.77	36.15	0.06	-2.35	-3.89	-59.42	0.18

💡 Note: The % column shows the percentage of members that CWNU 4205 shares with each listed object.

Visualization

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