CWNU 1464

0.24 UTI

0.0

C_N

0.19

C_dens

0.38

C_C3

0.31

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 22

Radius (P>50% members) 11.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.19 Very loose
C_C3 0.38 Low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

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CWNU 1464 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1464 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	–	85.124	32.014	0.728	-0.116	-3.006	12.638
Zhang et al.	2024	85.142	31.841	–	–	–	–
Hunt & Reffert	2024	85.142	31.841	0.721	-0.096	-3.026	12.569
Cavallo et al.	2024	85.367	32.182	0.72	–	–	–
Hunt & Reffert	2023	85.142	31.841	0.721	-0.096	-3.026	12.569
He et al.	2023	85.129	32.111	0.737	-0.101	-2.99	–

💡 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
Zhang et al.	2024	–	–	–	–	0.005*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	53*	–	–
Cavallo et al.	2024	1.32	1.34	–	22	-0.330	–	–	–
Hunt & Reffert	2023	1.27	0.97	1.92	56	–	–	–	–
He et al.	2023	1.41	1.45	–	13	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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