CWNU 1465

0.57 UTI

0.43

C_N

1.0

C_dens

1.0

C_C3

0.25

C_lit

0.98

C_dup

C3 classification AA

Number of members (P>50%) 43

Radius (P>50% members) 2.4 [arcmin]

C_N 0.43 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.25 Poorly studied
C_dup 0.98 Unique

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

Overview

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CWNU 1465 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High extinction Metal-poor Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1465 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	–	270.365	-23.543	0.339	-0.439	-1.635	22.07
Hunt & Reffert	2024	270.365	-23.546	0.346	-0.42	-1.61	–
Cavallo et al.	2024	270.362	-23.528	0.346	–	–	–
Hunt & Reffert	2023	270.365	-23.546	0.346	-0.42	-1.61	–
He et al.	2023	270.362	-23.532	0.358	-0.44	-1.626	–

💡 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	–	–	–	–	–	541*	–	–
Cavallo et al.	2024	1.58	3.31	–	55	-0.590	–	–	–
Hunt & Reffert	2023	2.63	2.98	1.44	15	–	–	–	–
He et al.	2023	2.45	3.20	–	32	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Ruprecht 139	2.3	270.23	-23.53	0.32	-0.01	-1.41	1.35	0.78

💡 Note: The % column shows the percentage of members that CWNU 1465 shares with each listed object.

Visualization

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