CWNU 1518

0.08 UTI

0.38

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.21

C_dup

C3 classification BB

Number of members (P>50%) 38

Radius (P>50% members) 1.2 [arcmin]

C_N 0.38 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.21 Likely duplicate

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

Overview

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CWNU 1518 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 very high extinction. It is catalogued as a young cluster (see Parameters). It was recently reported 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.

Distant Very high extinction Young

Data

🔍 Search references for CWNU 1518 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	–	287.356	10.334	0.262	-1.364	-3.632	97.191
He et al.	2023	287.353	10.334	0.271	-1.364	-3.638	40.72

💡 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	3.39	5.25	–	56	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Juchert 2	78.9	287.36	10.33	0.26	-1.37	-3.64	97.19	0.46

💡 Note: The % column shows the percentage of members that CWNU 1518 shares with each listed object.

Visualization

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