CWNU 3467

0.31 UTI

0.38

C_N

0.93

C_dens

0.25

C_C3

0.0

C_lit

1.0

C_dup

C3 classification DB

Number of members (P>50%) 38

Radius (P>50% members) 1.3 [arcmin]

C_N 0.38 Poorly populated
C_dens 0.93 Very dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 3467 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~7.56 kpc) differs significantly from the median photometric distance (~5.62 kpc).

Very distant Moderate extinction Old

Data

🔍 Search references for CWNU 3467 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	–	163.263	-57.501	0.132	-5.537	2.458	15.684
He et al.	2023	163.263	-57.498	0.129	-5.535	2.454	15.68

💡 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	5.62	1.60	–	1000	–	–	–	–

Visualization

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