CWNU 3245

0.07 UTI

0.35

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.17

C_dup

N₅₀ (P>50% members) 35

Stellar density (N₅₀/rad) 7.3 [N/pc²]

C3 classification AB

C_N 0.35 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.17 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3245 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate 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.

Very distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3245 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–	86.996	25.501	0.159	0.34	-0.422	15.534
He et al.	2023	86.995	25.505	0.166	0.345	-0.417	–

💡 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–	6.76	2.1	–	251	–	–	–	–
He et al.	2023	6.76	2.10	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 57	82.9	87.0	25.5	0.17	0.33	-0.41	30.65	0.42

💡 Note: The % column shows the percentage of members that CWNU 3245 shares with each listed object.

Visualization

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