CWNU 4265

0.09 UTI

0.55

C_N

0.16

C_dens

0.12

C_C3

0.0

C_lit

0.54

C_dup

C3 classification DC

Number of members (P>50%) 59

Radius (P>50% members) 4.9 [arcmin]

C_N 0.55 Moderately populated
C_dens 0.16 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.54 Likely unique

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

Overview

ℹ️

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.

(*): The parallax distance estimate (~6.05 kpc) differs significantly from the median photometric distance (~4.47 kpc).

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

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	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]	Bfr	BSS
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

ℹ️