CWNU 375

0.30 UTI

0.27

C_N

0.58

C_dens

0.75

C_C3

0.0

C_lit

0.93

C_dup

C3 classification BA

Number of members (P>50%) 27

Radius (P>50% members) 31.1 [arcmin]

C_N 0.27 Poorly populated
C_dens 0.58 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.93 Very likely unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 375 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It is rarely studied in the literature.

Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Metal-rich Young

Data

🔍 Search references for CWNU 375 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	–	285.569	41.633	2.958	1.62	-1.177	-21.359
He et al.	2022	286.14	41.582	2.94	1.65	-1.13	-18.3

💡 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]	Bfr	BSS
He et al.	2022	0.35	0.06	–	32	0.805	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 101	7.4	284.76	39.8	2.84	1.39	-1.74	-19.17	0.53

💡 Note: The % column shows the percentage of members that CWNU 375 shares with each listed object.

Visualization

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