CWNU 1467

0.32 UTI

0.34

C_N

0.51

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 34

Stellar density (N₅₀/rad) 2.5 [N/pc²]

C3 classification AB

C_N 0.34 Poorly populated
C_dens 0.51 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1467 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 1467 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	99999–	264.646	-33.675	0.539	0.386	-0.4	10.019
Hunt & Reffert	2024	264.673	-33.698	0.54	0.385	-0.376	–
Hunt & Reffert	2023	264.673	-33.698	0.54	0.385	-0.376	–
He et al.	2023	264.644	-33.689	0.543	0.388	-0.397	–

💡 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–	1.755	2.66	1.89	297	–	339	–	–
Hunt & Reffert	2024	–	–	–	–	–	339⁽¹⁾	–	–
Hunt & Reffert	2023	1.73	2.62	1.89	93	–	–	–	–
He et al.	2023	1.78	2.70	–	501	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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