CWNU 107

0.30 UTI

0.35

C_N

0.39

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 35

Stellar density (N₅₀/rad) 2.0 [N/pc²]

C3 classification AB

C_N 0.35 Poorly populated
C_dens 0.39 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 107 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a very metal-poor, young cluster (see Parameters). It is rarely studied in the literature.

Very close Low extinction Very metal-poor Young

Data

🔍 Search references for CWNU 107 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–	90.684	-17.407	3.713	-5.421	6.49	22.201
He et al.	2022	90.872	-17.248	3.88	-5.33	6.76	19.9

💡 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–	0.23	0.06	–	20	-1.335	–	–	–
He et al.	2022	0.23	0.06	–	20	-1.335	–	–	–

Visualization

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