CWNU 3672

0.09 UTI

0.49

C_N

0.53

C_dens

0.75

C_C3

0.0

C_lit

0.26

C_dup

C3 classification AB

Number of members (P>50%) 49

Radius (P>50% members) 2.4 [arcmin]

C_N 0.49 Poorly populated
C_dens 0.53 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.26 Possibly duplicate

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

Overview

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CWNU 3672 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a large distance, well above 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 possibly a duplicate object, which shares a significant 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 3672 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	–	50.088	65.072	0.162	-0.306	0.164	-72.194
He et al.	2023	50.092	65.067	0.163	-0.305	0.166	–

💡 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	5.62	2.80	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1117	73.5	50.1	65.07	0.16	-0.31	0.16	–	0.33

💡 Note: The % column shows the percentage of members that CWNU 3672 shares with each listed object.

Visualization

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