CWNU 360

0.30 UTI

0.4

C_N

0.23

C_dens

0.75

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 40

Core radius and density 1.7 [pc], 1.2 [pc^-2]

C3 classification AB

C_N 0.4 Poorly populated
C_dens 0.23 Very loose
C_C3 0.75 High quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 360 is a poorly populated, very loose object of 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-rich, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is rarely studied in the literature.

Relatively close High extinction Metal-rich Young

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.65 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.65 (50th percentile).

Data

🔍 Search references for CWNU 360 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–	234.506	-57.091	0.386	-3.604	-2.669	14.079
Hunt & Reffert	2024	234.538	-57.094	0.391	-3.563	-2.676	15.57
Cavallo et al.	2024	234.517	-57.088	0.386	–	–	–
Hunt & Reffert	2023	234.538	-57.094	0.391	-3.563	-2.676	15.57
He et al.	2022	234.53	-57.082	0.39	-3.6	-2.68	–

💡 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–	2.38	4.035	2.02	88	0.625	568	–	–
Hunt & Reffert	2024	2.38	4.38	2.02	70	–	568⁽¹⁾	–	–
Cavallo et al.	2024	2.61	3.69	–	107	0.830	–	–	–
Hunt & Reffert	2023	2.38	4.38	2.02	70	–	–	–	–
He et al.	2022	2.09	3.68	–	501	0.420	–	–	–

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

Visualization

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