CWNU 150

0.10 UTI

0.5

C_N

0.51

C_dens

0.75

C_C3

0.0

C_lit

0.28

C_dup

N₅₀ (P>50% members) 50

Stellar density (N₅₀/rad) 2.6 [N/pc²]

C3 classification AB

C_N 0.5 Moderately populated
C_dens 0.51 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 150 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Metal-rich Young

Data

🔍 Search references for CWNU 150 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–	119.743	-40.137	0.552	-4.121	4.793	14.4
He et al.	2022	119.755	-40.112	0.55	-4.12	4.79	–

💡 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–	1.95	1.8	–	25	0.537	–	–	–
He et al.	2022	1.95	1.80	–	25	0.537	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0448	72.0	119.75	-40.13	0.55	-4.14	4.79	–	0.4

💡 Note: The % column shows the percentage of members that CWNU 150 shares with each listed object.

Visualization

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