CWNU 3267

0.05 UTI

0.61

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.11

C_dup

C3 classification BA

Number of members (P>50%) 72

Radius (P>50% members) 1.4 [arcmin]

C_N 0.61 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.11 Likely duplicate

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

Overview

ℹ️

CWNU 3267 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

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

(*): The parallax distance estimate (~7.02 kpc) differs significantly from the median photometric distance (~4.90 kpc).

Distant Moderate extinction Old

Data

🔍 Search references for CWNU 3267 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	200.909	-63.67	0.142	-6.348	-1.01	-11.987
He et al.	2023	200.907	-63.669	0.142	-6.344	-1.024	-11.99

💡 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	4.90	2.70	–	1585	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 79	88.9	200.91	-63.67	0.14	-6.35	-1.01	-11.99	0.65

💡 Note: The % column shows the percentage of members that CWNU 3267 shares with each listed object.

Visualization

ℹ️