CWNU 1495

0.36 UTI

0.38

C_N

0.17

C_dens

0.75

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 38

Stellar density (N₅₀/rad) 0.9 [N/pc²]

C3 classification AB

C_N 0.38 Poorly populated
C_dens 0.17 Very loose
C_C3 0.75 High quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1495 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Distant Low extinction Metal-rich Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1495 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–	117.236	-21.149	0.26	-1.845	2.491	–
Hunt & Reffert	2024	117.222	-21.203	0.261	-1.858	2.489	–
Cavallo et al.	2024	117.227	-21.149	0.265	–	–	–
Hunt & Reffert	2023	117.222	-21.203	0.261	-1.858	2.489	–
He et al.	2023	117.264	-21.153	0.268	-1.853	2.483	–

💡 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–	3.33	0.85	0.72	113	0.530	145	–	–
Hunt & Reffert	2024	–	–	–	–	–	145⁽¹⁾	–	–
Cavallo et al.	2024	3.25	0.37	–	219	0.530	–	–	–
Hunt & Reffert	2023	3.33	0.85	0.72	113	–	–	–	–
He et al.	2023	3.89	1.10	–	32	–	–	–	–

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

Visualization

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