CWNU 1148

0.31 UTI

0.35

C_N

0.7

C_dens

0.5

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 35

Radius (P>50% members) 10.5 [arcmin]

C3 classification BB

C_N 0.35 Poorly populated
C_dens 0.7 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 1148 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Moderate extinction Young

Data

🔍 Search references for CWNU 1148 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	–	315.039	38.992	0.963	-3.275	-8.957	-14.924
He et al.	2022	315.044	39.0	0.962	-3.271	-8.947	–

💡 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
He et al.	2022	–	1.25	–	45	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 3916	100.0	315.1	38.99	0.96	-3.28	-8.96	-15.5	0.2

💡 Note: The % column shows the percentage of members that CWNU 1148 shares with each listed object.

Visualization

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