CWNU 4248

0.02 UTI

0.0

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.08

C_dup

C3 classification CB

Number of members (P>50%) 24

Radius (P>50% members) 2.1 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

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

Overview

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CWNU 4248 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate^* distance, below 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 very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~3.51 kpc) differs significantly from the median photometric distance (~2.69 kpc).

Relatively close High extinction Very young

Data

🔍 Search references for CWNU 4248 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	–	298.896	25.018	0.285	-2.626	-6.346	–
He et al.	2023	298.9	25.01	0.292	-2.626	-6.322	–

💡 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	2.69	4.20	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 504	92.0	298.9	25.02	0.29	-2.63	-6.35	–	0.24

💡 Note: The % column shows the percentage of members that CWNU 4248 shares with each listed object.

Visualization

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