CWNU 1006

0.34 UTI

0.34

C_N

0.75

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

C3 classification CA

Number of members (P>50%) 34

Radius (P>50% members) 31.0 [arcmin]

C_N 0.34 Poorly populated
C_dens 0.75 Dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 1006 is a poorly populated, dense 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.

Note: This object shares a large percentage of members with a later 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	–	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]	Bfr	BSS
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	0.0

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

Visualization

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