CWNU 1894

0.38 UTI

0.28

C_N

0.37

C_dens

0.75

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 28

Stellar density (N₅₀/rad) 1.9 [N/pc²]

C3 classification BA

C_N 0.28 Poorly populated
C_dens 0.37 Loose
C_C3 0.75 High quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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CWNU 1894 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Very distant Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1894 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–	41.937	63.031	0.143	-0.798	0.449	–
Hunt & Reffert	2024	41.955	63.032	0.145	-0.799	0.435	–
Cavallo et al.	2024	41.908	63.029	0.147	–	–	–
Hunt & Reffert	2023	41.955	63.032	0.145	-0.799	0.435	–
He et al.	2023	41.908	63.039	0.149	-0.798	0.408	–

💡 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–	7.33	2.76	1.51	43	0.200	642	–	–
Hunt & Reffert	2024	–	–	–	–	–	642⁽¹⁾	–	–
Cavallo et al.	2024	5.52	2.50	–	26	0.200	–	–	–
Hunt & Reffert	2023	7.33	2.76	1.51	43	–	–	–	–
He et al.	2023	7.76	3.00	–	50	–	–	–	–

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

Visualization

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