CWNU 4148

0.12 UTI

0.41

C_N

0.22

C_dens

0.75

C_C3

0.0

C_lit

0.44

C_dup

C3 classification AB

Number of members (P>50%) 41

Radius (P>50% members) 2.9 [arcmin]

C_N 0.41 Poorly populated
C_dens 0.22 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

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

Overview

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CWNU 4148 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large distance, below 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 4148 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	–	113.026	-24.7	0.137	-0.772	1.409	73.597
He et al.	2023	113.028	-24.702	0.137	-0.775	1.425	67.6

💡 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	6.76	2.50	–	200	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1914	56.1	113.04	-24.71	0.14	-0.77	1.39	87.43	0.1

💡 Note: The % column shows the percentage of members that CWNU 4148 shares with each listed object.

Visualization

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