CWNU 1592

0.37 UTI

0.37

C_N

1.0

C_dens

0.12

C_C3

0.25

C_lit

0.92

C_dup

N₅₀ (P>50% members) 37

Stellar density (N₅₀/rad) 6.8 [N/pc²]

C3 classification DC

C_N 0.37 Poorly populated
C_dens 1.0 Very dense
C_C3 0.12 Very low quality
C_lit 0.25 Poorly studied
C_dup 0.92 Very likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1592 is a poorly populated, very dense object of very low C3 quality. Its parallax locates it at a moderate distance, below 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 age parameter (see Parameters). It was recently reported in the literature.

Note: This is very likely 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 Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1592 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–	112.668	-23.148	0.323	-1.76	1.723	–
Hunt & Reffert	2024	112.682	-23.148	0.328	-1.768	1.712	–
Cavallo et al.	2024	112.675	-23.153	0.328	–	–	–
Hunt & Reffert	2023	112.682	-23.148	0.328	-1.768	1.712	–
He et al.	2023	112.661	-23.157	0.325	-1.721	1.727	84.98

💡 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–	2.99	2.2	1.33	59	0.000	252	–	–
Hunt & Reffert	2024	–	–	–	–	–	252⁽¹⁾	–	–
Cavallo et al.	2024	3.24	2.33	–	59	0.000	–	–	–
Hunt & Reffert	2023	2.99	1.91	1.33	52	–	–	–	–
He et al.	2023	2.82	2.20	–	501	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Ruprecht 23	8.1	112.66	-23.38	0.34	-2.06	1.61	59.89	0.91

💡 Note: The % column shows the percentage of members that CWNU 1592 shares with each listed object.

Visualization

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