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

C3 classification AB

Number of members (P>50%) 34

Radius (P>50% members) 6.8 [arcmin]

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

Overview

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 (see Parameters). It was recently reported in the literature.

Relatively close Moderate extinction Intermediate age

Data

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	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]	Bfr	BSS
Hunt & Reffert	2024	–	–	–	–	–	339*	–	–
Hunt & Reffert	2023	1.73	2.62	1.89	93	–	–	–	–
He et al.	2023	1.78	2.70	–	501	–	–	–	–

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

1 2

💡 Note: How are the galactocentric plots generated? See FAQ.