CWNU 1417

0.03 UTI

0.3

C_N

0.28

C_dens

0.62

C_C3

0.0

C_lit

0.13

C_dup

C3 classification CA

Number of members (P>50%) 30

Radius (P>50% members) 2.5 [arcmin]

C_N 0.3 Poorly populated
C_dens 0.28 Loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.13 Likely duplicate

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

Overview

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CWNU 1417 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a large 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 1417 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	–	165.205	-61.621	0.157	-6.072	2.52	23.421
He et al.	2023	165.2	-61.629	0.161	-6.072	2.509	24.34

💡 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	5.37	1.55	–	447	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch J1059.7-6131	86.7	165.11	-61.59	0.14	-6.1	2.54	24.22	0.3

💡 Note: The % column shows the percentage of members that CWNU 1417 shares with each listed object.

Visualization

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