CWNU 4175

0.19 UTI

0.55

C_N

0.33

C_dens

0.75

C_C3

0.0

C_lit

0.58

C_dup

N₅₀ (P>50% members) 59

Stellar density (N₅₀/rad) 1.6 [N/pc²]

C3 classification AB

C_N 0.55 Moderately populated
C_dens 0.33 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 4175 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very young 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.

Relatively close Moderate extinction Very young

Data

🔍 Search references for CWNU 4175 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–	354.571	68.496	0.948	-2.393	-2.939	-11.413
He et al.	2023	354.603	68.525	0.948	-2.405	-2.942	-3.3

💡 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–	1.02	2.55	–	13	–	–	–	–
He et al.	2023	1.02	2.55	–	13	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 925	42.4	354.77	68.54	0.95	-2.38	-2.92	-6.44	0.19

💡 Note: The % column shows the percentage of members that CWNU 4175 shares with each listed object.

Visualization

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