CWNU 1351

0.02 UTI

0.0

C_N

0.62

C_dens

0.75

C_C3

0.0

C_lit

0.08

C_dup

C3 classification BA

Number of members (P>50%) 21

Radius (P>50% members) 1.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.62 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

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

Overview

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CWNU 1351 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a large distance, below 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 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.

Very distant High extinction Very young

Data

🔍 Search references for CWNU 1351 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	–	201.419	-63.452	0.123	-6.948	-1.136	-38.099
He et al.	2023	201.428	-63.449	0.123	-6.952	-1.144	–

💡 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	7.08	3.15	–	8	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Ruprecht 166	92.0	201.42	-63.46	0.12	-6.94	-1.13	-38.1	0.48

💡 Note: The % column shows the percentage of members that CWNU 1351 shares with each listed object.

Visualization

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