CWNU 4265

0.08 UTI

0.55

C_N

0.05

C_dens

0.12

C_C3

0.0

C_lit

0.54

C_dup

N_m (P>50%) 59

Core radius and density 4.6 [pc], 0.3 [pc^-2]

C3 classification DC

C_N 0.55 Moderately populated
C_dens 0.05 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.54 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 4265 is a moderately populated, very loose object of very low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a 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.

Distant Moderate extinction Young

Data

🔍 Search references for CWNU 4265 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–	102.69	-3.589	0.165	-0.535	0.922	90.75
He et al.	2023	102.69	-3.591	0.168	-0.54	0.922	–

💡 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–	4.47	2.45	–	20	–	–	–	–
He et al.	2023	4.47	2.45	–	20	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1706	45.8	102.69	-3.61	0.17	-0.51	0.9	105.34	0.18

💡 Note: The % column shows the percentage of members that CWNU 4265 shares with each listed object.

Visualization

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