CWNU 1356

0.36 UTI

0.31

C_N

0.24

C_dens

0.75

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 31

Stellar density (N₅₀/rad) 1.2 [N/pc²]

C3 classification AB

C_N 0.31 Poorly populated
C_dens 0.24 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 1356 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 low extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

Relatively close Low extinction Metal-rich Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1356 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–	170.438	-60.879	0.367	-5.873	0.75	-64.337
Hunt & Reffert	2024	170.389	-60.887	0.373	-5.863	0.791	-64.294
Cavallo et al.	2024	170.461	-60.869	0.37	–	–	–
Hunt & Reffert	2023	170.389	-60.887	0.373	-5.863	0.791	-64.294
He et al.	2023	170.393	-60.881	0.368	-5.885	0.75	–

💡 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–	2.47	0.97	0.94	26	0.790	319	–	–
Hunt & Reffert	2024	–	–	–	–	–	319⁽¹⁾	–	–
Cavallo et al.	2024	2.47	0.76	–	59	0.790	–	–	–
Hunt & Reffert	2023	2.43	0.97	0.94	26	–	–	–	–
He et al.	2023	2.57	1.20	–	14	–	–	–	–

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

Visualization

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