CWNU 3248

0.06 UTI

0.56

C_N

0.35

C_dens

0.38

C_C3

0.0

C_lit

0.25

C_dup

C3 classification CB

Number of members (P>50%) 61

Radius (P>50% members) 4.1 [arcmin]

C_N 0.56 Moderately populated
C_dens 0.35 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.25 Possibly duplicate

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

Overview

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CWNU 3248 is a moderately populated, loose object of low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by high extinction. It is catalogued as a very young 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.

(*): The parallax distance estimate (~4.93 kpc) differs significantly from the median photometric distance (~9.33 kpc).

Very distant High extinction Very young

Data

🔍 Search references for CWNU 3248 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	–	323.267	51.315	0.203	-3.357	-3.34	-65.81
He et al.	2023	323.277	51.32	0.201	-3.328	-3.341	–

💡 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	9.33	4.70	–	5	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 739	75.4	323.27	51.31	0.2	-3.35	-3.34	–	0.23

💡 Note: The % column shows the percentage of members that CWNU 3248 shares with each listed object.

Visualization

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