CWNU 1486

0.02 UTI

0.0

C_N

0.52

C_dens

0.25

C_C3

0.0

C_lit

0.12

C_dup

N₅₀ (P>50% members) 17

Stellar density (N₅₀/rad) 2.6 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.52 Moderately dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1486 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very 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.

Relatively close High extinction Very young

Data

🔍 Search references for CWNU 1486 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–	58.043	52.489	0.434	0.86	-1.584	–
He et al.	2023	58.049	52.481	0.443	0.853	-1.584	–

💡 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–	2.14	3.1	–	18	–	–	–	–
He et al.	2023	2.14	3.10	–	18	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 194	88.0	58.04	52.49	0.43	0.89	-1.56	–	0.29

💡 Note: The % column shows the percentage of members that CWNU 1486 shares with each listed object.

Visualization

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