CWNU 4162

0.07 UTI

0.3

C_N

0.07

C_dens

0.75

C_C3

0.0

C_lit

0.33

C_dup

N_m (P>50%) 30

Core radius and density 2.4 [pc], 0.3 [pc^-2]

C3 classification AB

C_N 0.3 Poorly populated
C_dens 0.07 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.33 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

CWNU 4162 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Young

Data

🔍 Search references for CWNU 4162 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	96.785	17.739	0.178	-0.064	-0.48	18.991
He et al.	2023	96.788	17.767	0.185	-0.099	-0.476	25.13

💡 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–	5.13	1.55	–	79	–	–	–	–
He et al.	2023	5.13	1.55	–	79	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1540	66.7	96.79	17.73	0.17	-0.06	-0.47	18.99	0.12

💡 Note: The % column shows the percentage of members that CWNU 4162 shares with each listed object.

Visualization

ℹ️