CWNU 2595

0.24 UTI

0.0

C_N

0.11

C_dens

0.5

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 21

Stellar density (N₅₀/rad) 0.6 [N/pc²]

C3 classification BB

C_N 0.0 Sparse
C_dens 0.11 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.3 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 2595 is a sparse, very loose object of intermediate 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, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 2595 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–	93.399	14.275	0.249	0.015	-0.705	–
Zhang et al.	2024	93.364	14.237	–	–	–	–
Hunt & Reffert	2024	93.364	14.237	0.248	0.038	-0.713	32.767
Cavallo et al.	2024	93.432	14.26	0.249	–	–	–
Hunt & Reffert	2023	93.364	14.237	0.248	0.038	-0.713	32.767
He et al.	2023	93.395	14.295	0.273	-0.011	-0.686	30.24

💡 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–	3.68	2.5	2.51	110	0.179	620	–	–
Zhang et al.	2024	–	–	–	–	-0.231⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	620⁽¹⁾	–	–
Cavallo et al.	2024	3.68	2.50	–	158	0.590	–	–	–
Hunt & Reffert	2023	3.48	2.37	2.51	110	–	–	–	–
He et al.	2023	4.68	3.05	–	71	–	–	–	–

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

Visualization

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