CWNU 3279

0.06 UTI

0.32

C_N

0.12

C_dens

0.75

C_C3

0.0

C_lit

0.25

C_dup

C3 classification AB

Number of members (P>50%) 32

Radius (P>50% members) 6.2 [arcmin]

C_N 0.32 Poorly populated
C_dens 0.12 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.25 Possibly duplicate

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

Overview

ℹ️

CWNU 3279 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age 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.

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3279 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	20.442	57.249	0.252	-2.125	-1.109	-62.619
He et al.	2023	20.454	57.249	0.256	-2.104	-1.087	-62.62

💡 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	3.98	1.25	–	501	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1021	75.0	20.54	57.24	0.26	-2.12	-1.09	-62.62	0.37

💡 Note: The % column shows the percentage of members that CWNU 3279 shares with each listed object.

Visualization

ℹ️