CWNU 1362

0.35 UTI

0.49

C_N

0.37

C_dens

0.75

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 49

Core radius and density 2.1 [pc], 1.9 [pc^-2]

C3 classification AB

C_N 0.49 Poorly populated
C_dens 0.37 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 1362 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Relatively close High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.91 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.91 (50th percentile).

Data

🔍 Search references for CWNU 1362 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–	228.876	-59.177	0.316	-4.324	-4.213	-147.628
Hunt & Reffert	2024	228.877	-59.177	0.316	-4.352	-4.2	-109.251
Cavallo et al.	2024	228.861	-59.178	0.318	–	–	–
Hunt & Reffert	2023	228.877	-59.177	0.316	-4.352	-4.2	-109.251
He et al.	2023	228.863	-59.17	0.316	-4.327	-4.208	–

💡 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–	2.82	3.465	1.92	103	0.050	969	–	–
Hunt & Reffert	2024	2.82	3.44	1.92	71	–	969⁽¹⁾	–	–
Cavallo et al.	2024	2.39	3.49	–	135	0.050	–	–	–
Hunt & Reffert	2023	2.82	3.44	1.92	71	–	–	–	–
He et al.	2023	2.82	3.55	–	141	–	–	–	–

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

Visualization

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