CWNU 3517

0.07 UTI

0.33

C_N

0.15

C_dens

0.62

C_C3

0.0

C_lit

0.3

C_dup

C3 classification AC

Number of members (P>50%) 33

Radius (P>50% members) 4.2 [arcmin]

C_N 0.33 Poorly populated
C_dens 0.15 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.3 Possibly duplicate

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

Overview

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CWNU 3517 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a young 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 Young

Data

🔍 Search references for CWNU 3517 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	–	88.344	36.136	0.185	-0.193	-0.85	–
He et al.	2023	88.335	36.144	0.198	-0.12	-0.853	–

💡 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	5.01	1.45	–	50	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1365	69.7	88.34	36.14	0.19	-0.24	-0.85	–	0.14

💡 Note: The % column shows the percentage of members that CWNU 3517 shares with each listed object.

Visualization

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