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

C3 classification BB

Number of members (P>50%) 29

Radius (P>50% members) 4.3 [arcmin]

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

Overview

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

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	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]	Bfr	BSS
He et al.	2023	2.88	3.20	–	316	–	–	–	–

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.

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

💡 Note: How are the galactocentric plots generated? See FAQ.