CWNU 1348

0.01 UTI

0.25

C_N

0.49

C_dens

0.62

C_C3

0.0

C_lit

0.04

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 2.4 [N/pc²]

C3 classification AC

C_N 0.25 Poorly populated
C_dens 0.49 Loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.04 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 1348 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate 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 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.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 1348 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	99999–	134.946	-52.675	0.462	-7.971	6.002	24.478
He et al.	2023	134.946	-52.698	0.46	-7.985	5.999	24.25

💡 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
UCC	99999–	2.04	1.5	–	891	–	–	–	–
He et al.	2023	2.04	1.50	–	891	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 1478	96.0	134.94	-52.67	0.46	-7.97	6.0	24.48	0.48

💡 Note: The % column shows the percentage of members that CWNU 1348 shares with each listed object.

Visualization

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