CWNU 1506

0.30 UTI

0.25

C_N

0.25

C_dens

0.5

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 1.3 [N/pc²]

C3 classification BB

C_N 0.25 Poorly populated
C_dens 0.25 Loose
C_C3 0.5 Intermediate 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 1506 is a poorly populated, 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, very young cluster (see Parameters). It was recently reported in the literature.

Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

🔍 Search references for CWNU 1506 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–	356.204	59.674	0.321	-2.721	-1.879	–
Hunt & Reffert	2024	356.136	59.673	0.326	-2.71	-1.88	–
Cavallo et al.	2024	356.187	59.663	0.326	–	–	–
Hunt & Reffert	2023	356.136	59.673	0.326	-2.71	-1.88	–
He et al.	2023	356.25	59.648	0.321	-2.721	-1.911	–

💡 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–	2.94	2.77	1.73	12	0.200	280	–	–
Hunt & Reffert	2024	–	–	–	–	–	280⁽¹⁾	–	–
Cavallo et al.	2024	2.94	2.51	–	23	0.200	–	–	–
Hunt & Reffert	2023	2.75	2.77	1.73	12	–	–	–	–
He et al.	2023	2.95	3.05	–	6	–	–	–	–

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

Visualization

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