CWNU 1006

0.05 UTI

0.34

C_N

0.21

C_dens

0.62

C_C3

0.0

C_lit

0.21

C_dup

N_m (P>50%) 34

Core radius and density 0.8 [pc], 1.1 [pc^-2]

C3 classification CA

C_N 0.34 Poorly populated
C_dens 0.21 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.21 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1006 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.

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

Low extinction Young

Data

🔍 Search references for CWNU 1006 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–	5.31	68.571	2.997	-6.658	0.119	-8.662
He et al.	2022	5.352	68.605	2.997	-6.617	0.144	–

💡 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–	–	0.75	–	71	–	–	–	–
He et al.	2022	–	0.75	–	71	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 698	79.4	5.25	68.59	3.0	-6.66	0.1	-8.85	0.19

💡 Note: The % column shows the percentage of members that CWNU 1006 shares with each listed object.

Visualization

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