CWNU 248

0.04 UTI

0.56

C_N

0.85

C_dens

0.5

C_C3

0.0

C_lit

0.12

C_dup

C3 classification BB

Number of members (P>50%) 61

Radius (P>50% members) 5.0 [arcmin]

C_N 0.56 Moderately populated
C_dens 0.85 Dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

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

Overview

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CWNU 248 is a moderately populated, dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied 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 Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CWNU 248 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	–	303.62	37.402	0.383	-1.304	-3.14	-3.403
He et al.	2022	303.61	37.4	0.38	-1.28	-3.14	-3.9

💡 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.	2022	2.40	2.16	–	251	0.370	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1097	88.5	303.63	37.41	0.37	-1.31	-3.15	-3.4	0.5
CWWDL 10236	75.4	303.62	37.41	0.38	-1.33	-3.16	-3.4	0.02

💡 Note: The % column shows the percentage of members that CWNU 248 shares with each listed object.

Visualization

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