CWNU 3207

0.02 UTI

0.29

C_N

0.31

C_dens

0.5

C_C3

0.0

C_lit

0.1

C_dup

N₅₀ (P>50% members) 29

Stellar density (N₅₀/rad) 1.5 [N/pc²]

C3 classification BB

C_N 0.29 Poorly populated
C_dens 0.31 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.1 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3207 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported 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.

Relatively close High extinction Intermediate age

Data

🔍 Search references for CWNU 3207 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–	103.502	-4.525	0.288	-0.706	0.621	–
He et al.	2023	103.512	-4.522	0.279	-0.709	0.617	–

💡 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–	2.88	3.2	–	316	–	–	–	–
He et al.	2023	2.88	3.20	–	316	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
ASCC 27	89.7	103.5	-4.5	0.28	-0.71	0.62	–	0.54
BDSB 88	75.9	103.55	-4.53	0.27	-0.73	0.67	–	0.1

💡 Note: The % column shows the percentage of members that CWNU 3207 shares with each listed object.

Visualization

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