CWNU 1404

0.02 UTI

0.36

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.06

C_dup

N₅₀ (P>50% members) 36

Stellar density (N₅₀/rad) 15.1 [N/pc²]

C3 classification BB

C_N 0.36 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.06 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1404 is a poorly populated, very 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 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.

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 1404 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–	95.591	21.244	0.301	-0.313	-0.126	31.482
He et al.	2023	95.597	21.248	0.304	-0.324	-0.115	31.48

💡 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–	3.24	1.65	–	316	–	–	–	–
He et al.	2023	3.24	1.65	–	316	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Alessi J0622.4+2114	94.4	95.59	21.24	0.3	-0.31	-0.12	31.48	0.54

💡 Note: The % column shows the percentage of members that CWNU 1404 shares with each listed object.

Visualization

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